FEMIS – Star Formation and Interstellar Medium

Star formation is the central process of the galactic cycle of matter and is at the origin of the formation of planetary systems. While simple in principle (gravitational collapse of an interstellar cloud of gas and dust), the details of the process are far from being well understood, especially for the most massive stars.

The star formation group at the LAB works on the physical processes leading to the formation and structuration of molecular clouds, the search for massive protostars, the role of the magnetic field, the search for complex molecules, and astrochemical processes during the massive star formation phase. In nearby galaxies, we address the question of the universality of the star formation process by probing a large range of physical conditions.

Structuration of the interstellar medium towards star formation

The star formation paradigm has recently shifted from a « gravo-turbulent » scenario with random occurrences of over-densities large enough to collapse, to a more dynamical view based on the formation of dense filaments prior to fragmentation in collapsing cores. The LAB group presently works on a better understanding of the origin of these star forming filaments thanks to new statistical tools developed by the GeoStat team from INRIA Bordeaux, and thanks to cooling lines observed with SOFIA (NASA-DLR stratospheric plane) in collaboration with the University of Cologne (ANR-DFG project GENESIS).

Our group is also involved in the preparation of the ESA-JAXA mission SPICA (cooled 2.5m spatial telescope) which will allow us to detect very weak cooling lines associated with the structuration of the interstellar medium.

Origin and formation of massive stars

High-mass star formation is not well explained with scenarios applying to low-mass star formation. The massive stars have masses significantly in excess of the typically observed Jeans masses in the interstellar medium. Our group is involved in ALMA programs (SPARKS and W43-HERO) aiming at recognizing the spetcal environments and conditions required to obtain Jeans masses comparable to the highest stellar masses. Resolving this issue may ultimately allow us to explain the origin of the upper limit for stellar masses (of the order of 100 to 150 Msun).

Astrochemistry in massive protostars

Astrochemistry provides a way to constrain the physical processes responsible for the formation of stars and, more importantly, the best way to evaluate to which extent complex molecules, especially those of prebiotic interest, are formed in the interstellar medium. Our team works on the origin and evolution of the « hot cores » (above 100 K) which are found within the collapsing envelopes of massive protostars. To this end, our team is also hunting for the rare complex molecules towards Orion KL, one of the two reference targets for such studies (SgrB2 being the second one). We plan to follow the chemical evolution of massive protostars to try to identify the dominant processes leading to the formation of complex molecules. Our work is primarily based on spectral surveys, some of them unbiased, obtained with ALMA, NOEMA and the IRAM 30m.

Stellar evolution and magnetic field

At the other end of the stellar life cycle, complex mass-loss processes dominate the evolution of a star when its nuclear fusion reactions have stopped. The dust and molecules formed at this stage enrich the interstellar medium. ALMA, APEX and the IRAM 30m are used to probe the chemistry, kinematics and mass losses of selected circumstellar envelopes (AGBs or supergiants).

The magnetic field plays a decisive role at several stages of the star evolution, from its formation to its most evolved stages. Our group works at characterizing the magnetic field in the evolved stages using Xpol on the IRAM 30m. Polarimetry with ALMA (and in a longer term with the instrument SAFARI-pol on SPICA) opens important perspectives to probe the magnetic field in protostellar and interstellar media for which sensitivity and spatial resolution are required.

Diversity and origin of star formation events in the local group

Nearby galaxies in the Local Group offer a unique opportunity to probe a significant range of galactic environments and conditions to test the universality of the star formation process, including structuration and formation of molecular clouds. Our group investigates for instance the relationship between the amount of dense gas and the star formation rate as well as the properties of the population of molecular clouds in nearby galaxies such as M33 (projects HerM33es and STARFICH).

Current members
Fabrice Herpin

Astronome CNAP

Theme leader

  • Formation of high-mass stars
  • Stellar evolution
  • Radio and IR spectroscopy (IRAM, Herschel, ALMA)
  • Line modeling (RATRAN, LIME)
  • Instrumentation (Herschel, SPICA)

Personal web page

Fabrice Herpin

Alain Baudry

Astronome CE, Prof. Emérite

• Interstellar and circumstellar medium

• Evolved stars and stars in formation

• Millimeter and submm interferometry, VLBI

• Correlator and back-end design for ALMA

Alain Baudry

Sylvain Bontemps

Directeur de recherche CNRS

• Formation of high-mass stars

• Protostars

• Structure of molecular clouds

• Millimeter interferometer (NOEMA and ALMA)

• Large FIR, submillimeter maps (Herschel, ATLASGAL)

Personnal web page

Sylvain Bontemps

Jonathan Braine

Astronome (CNAP)

• Extragalactic astrophysics

• Interstellar medium, molecular spectroscopy

• Millimeter interferometry (NOEMA et ALMA)

• Large imaging surveys (Herschel, IRAM)

Jonathan Braine

Nathalie Brouillet

Astronome adjoint (CNAP)

• Interstellar medium

• Complex molecules

• Millimeter interferometry

Nathalie Brouillet

Timea Csengeri

CNRS researcher

 • Galactic surveys
 • Massive star formation
 • mm and submm interferometry
 • THz Spectroscopy

Timea Csengeri

Pierre Gratier

Associate astronomer • Interstellar Medium • Local Group galaxies • Millimeter wave radio observations • Astrostatistics

Pierre Gratier

Thierry Jacq

Astronome adjoint

Formation of high-mass stars

Thierry Jacq

David Smith

Directeur de Recherche CNRS

  • Gamma ray pulsars, with the Large Area Telescope (LAT) on Fermi.
  • Radio ephemerides of pulsar rotation.
  • High energy cosmic phenomena.

David Smith

Valentine Wakelam

CNRS senior rechearcher

• Chemical modeling

• Cold cores, protostars and protoplanetary disks

Personal web page

Valentine Wakelam

Maxime Valeille-Manet

PhD student

  • Astrochemistry of massive and intermediate mass prestellar cores
  • Massive star formation scenarios

Maxime Valeille-Manet

Louise Marinho

PhD student

  • Evolved stars

Louise Marinho

Aimie Clément

Aimie Clément

Nina Kessler

Nina Kessler

Old members
Alizée Duthu

PhD student

• Magnetic fields

• Evolved stars

• Radio-astronomy

Alizée Duthu

Jordan Molet

PhD Student

• Search for complex molecules

• Millimeter interferometry (ALMA)

Jordan Molet

Arabindo Roy

Postdoc

• Galactic star formation

• Role of filaments in core formation

• Interstellar medium

• Interstellar dust evolution

Arabindo Roy

Mélisse BONFAND

Postdoc

  • Highmass star formation
  • Complex organic molecules
  • Mm & submm interferometry (ALMA)
  • Chemical modelling

Mélisse BONFAND

Sami DIB

Postdoc
  • Theoretical/numerical models
  • The stellar initial mass function
  • Star formation scaling laws
  • Structure of molecular clouds

Personal web page

Sami DIB

Lars Bonne

PhD student

  • Formation of dense molecular cores
  •  Massive star formation
  •  Search for low velocity shocks
  •  Astrochimistry of massive pre-stellar cores

Lars Bonne

Didier Despois

Chargé de recherche CNRS

• Complex and prebiotic molecules in the interstellar medium

• Orion KL

• Link with comets

• Exobiology

Didier Despois

Angèle Taillard

PhD student

  • Early phases of star formation
  • Astrochemistry
  • mm and submm observations

Angèle Taillard

Karlis Dzenis

PhD student

  • Evolved start
  • Laboratory astrophysics

Karlis Dzenis

Axis 1: The formation and astrochemistry of massive protostars
To understand the molecular composition of the envelopes of massive protostars, the team is involved in millimeter interferometric projects mainly with ALMA and NOEMA to explore the molecular composition of massive envelopes at an angular resolution of ~1000-2000 u.a. With ALMA, NOEMA and probably with SKA, a systematic search for complex molecules (COMs) in star forming regions will be conducted, in particular to constrain their origin, related to grain chemistry and/or accretion shocks. The IdEX Junior Chair project at UB, C-ORIGINS, thus aims to focus on the distribution and diversity of COMs towards massive protostars. The team is also strongly involved in the Large ALMA-IMF Program, which aims to count the population of proto-stars in a sample of Galactic proto-clusters, to study the evolution of the CMF and to understand the origin of the IMF. Complementary work towards Orion BN-KL, as well as studies in the Magellanic Clouds will be conducted.  
A special effort is planned to participate in the development of automatic methods for extracting information from wide or unbiased spectral surveys to proto-stars. We will also work on 2D and 3D modeling (lines and continuum).

Axis 2 : Formation and astrochemistry of the interstellar medium
The problem of star formation is turning more and more towards understanding the formation of dense structures (filaments, dense cores, massive ridges, massive dense cores, "hubs") that fragment into protostars. The formation of these dense structures can be related to the scenarios of formation of molecular complexes from atomic gas and to the global equilibrium of the cold interstellar medium (ISM). It is during the formation of these clouds and dense structures that the initial conditions of astrochemistry are set up. The diffuse ISM from which dense structures emerge is under various influences that are poorly understood: UV radiation, cosmic rays, magnetic field, turbulence and dissipation, shocks ... We will also study the properties of molecular clouds in various environments by comparing more distant objects to closer and thus better resolved objects.

Axis 3 : Evolved stars and interstellar enrichment
We will continue our multi-instrument study in the framework of the ANR PEPPER (https://lagrange.oca.eu/fr/welcome-to-anr-pepper) and the LP ALMA-ATOMIUM (https://fys.kuleuven.be/ster/research-projects/aerosol/atomium/atomium) in order to obtain an overview of the physical processes (especially the magnetic field) at work from the sub-photospheric layers to the circumstellar environment of evolved stars. Our goal is to better understand the dynamics and chemistry of the gas phase, the formation of dust in the winds and thus the phenomena of mass loss, and consequently the interstellar enrichment. In connection with these projects, the ANR WaterStars (LAB-ISM-IPAG collaboration) aims to study the ro-vibrational excitation of water in evolved stars (in particular for maser emissions). The aim is to obtain new collision data (ro-vibrational cross sections and rates) through new calculations and experiments, and then to exploit them in an advanced model of radiative transfer of water.
Part of the research on these objects will concern massive stars that have evolved to the pulsar stage (based on observations with Fermi LAT, Nançay, MeerKAT and eventually SKA) in order to better understand their physics, notably by exploiting the numerous gamma pulsar detections, thus allowing to better estimate their contribution to the diffuse Gamma emission, or to determine the mechanisms at the origin of high-energy cosmic rays in pulsar wind nebulae.


Year Publication Link
2023L. Ramambason, Vianney Lebouteiller, S. C. Madden, F. Galliano, C. T. Richardson, et al.. Modeling the molecular gas content and CO-to-H 2 conversion factors in low-metallicity star-forming dwarf galaxies. Astronomy and Astrophysics - A&A, 2023, 681, pp.A14. ⟨10.1051/0004-6361/202347280⟩. ⟨hal-04409896⟩Link
2023L. Ramambason, Vianney Lebouteiller, S. C. Madden, F. Galliano, C. T. Richardson, et al.. Modeling the molecular gas content and CO-to-H2 conversion factors in low-metallicity star-forming dwarf galaxies. 2023. ⟨hal-04301630⟩Link
2023A. C. Lanzafame, E. Brugaletta, Y. Frémat, R. Sordo, O. L. Creevey, et al.. Gaia Data Release 3. Stellar chromospheric activity and mass accretion from Ca II IRT observed by the Radial Velocity Spectrometer. Astronomy and Astrophysics - A&A, 2023, 674, pp.A30. ⟨10.1051/0004-6361/202244156⟩. ⟨hal-04072603⟩Link
2022N. Schneider, V. Ossenkopf-Okada, S. Clarke, R. S. Klessen, S. Kabanovic, et al.. Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds. 2022. ⟨hal-03799824⟩Link
2022S. A. Dzib, A. Y. Yang, J. S. Urquhart, S. -N. X. Medina, A. Brunthaler, et al.. GLOSTAR -- Radio Source Catalog II: $28^\circ < \ell < 36^\circ$ and $|b| < 1^\circ$, VLA B-configuration. 2022. ⟨hal-03799776⟩Link
2022N. Brouillet, D. Despois, J. Molet, T. Nony, F. Motte, et al.. ALMA-IMF. IV. A comparative study of the main hot cores in W43-MM1: Detection, temperature, and molecular composition. Astronomy and Astrophysics - A&A, 2022, 665 (2), pp.A140. ⟨10.1051/0004-6361/202243669⟩. ⟨hal-03799994⟩Link
2022K. Neralwar, D. Colombo, A. Duarte-Cabral, J. Urquhart, M. Mattern, et al.. The SEDIGISM survey: Molecular cloud morphology. Astronomy and Astrophysics - A&A, 2022, 664, pp.A84. ⟨10.1051/0004-6361/202142513⟩. ⟨hal-03799782⟩Link
2022L. Bouscasse, T. Csengeri, A. Belloche, F. Wyrowski, S. Bontemps, et al.. Sulphur-rich cold gas around the hot core precursor G328.2551-0.5321. Astronomy and Astrophysics - A&A, 2022, 662, pp.A32. ⟨10.1051/0004-6361/202140519⟩. ⟨hal-03799832⟩Link
2022N. Hambly, R. Andrae, F. de Angeli, M. Antonio, F. Arenou, et al.. Gaia DR3 documentation Chapter 20: Datamodel description. 2022. ⟨hal-03969804⟩Link
2022A. Yang, J. Urquhart, F. Wyrowski, M. Thompson, C. König, et al.. The SEDIGISM survey: A search for molecular outflows. Astronomy and Astrophysics - A&A, 2022, 658, pp.A160. ⟨10.1051/0004-6361/202142039⟩. ⟨hal-03799846⟩Link
2022Y. Lin, F. Wyrowski, H. Liu, A. Izquierdo, T. Csengeri, et al.. The evolution of temperature and density structures of OB cluster-forming molecular clumps. Astronomy and Astrophysics - A&A, 2022, 658, pp.A128. ⟨10.1051/0004-6361/202142023⟩. ⟨hal-03799850⟩Link
2022T. Csengeri, F. Wyrowski, K. M. Menten, H. Wiesemeyer, R. Güsten, et al.. SOFIA/GREAT observations of OD and OH rotational lines towards high-mass star forming regions. Astronomy and Astrophysics - A&A, 2022, 658, pp.A193. ⟨10.1051/0004-6361/202140577⟩. ⟨hal-03588498⟩Link
2022Frédérique Motte, Sylvain Bontemps, Timéa Csengeri, Yohan Pouteau, Fabien Louvet, et al.. ALMA-IMF. I. Investigating the origin of stellar masses: Introduction to the Large Program and first results. Astronomy and Astrophysics - A&A, 2022, 662, pp.A8. ⟨10.1051/0004-6361/202141677⟩. ⟨hal-03683790⟩Link
2021D. Colombo, A. Duarte-Cabral, A. R. Pettitt, J. S. Urquhart, F. Wyrowski, et al.. The SEDIGISM survey: The influence of spiral arms on the molecular gas distribution of the inner Milky Way. 2021. ⟨insu-03439581⟩Link
2021V. Veena, P. Schilke, Á. Sánchez-Monge, R. Klessen, F. Schuller, et al.. A Kiloparsec-scale Molecular Wave in the Inner Galaxy: Feather of the Milky Way?. The Astrophysical journal letters, 2021, 921 (2), pp.L42. ⟨10.3847/2041-8213/ac341f⟩. ⟨insu-03439558⟩Link
2021S. Suri, H. Beuther, C. Gieser, A. Ahmadi, Á. Sánchez-Monge, et al.. Disk fragmentation in high-mass star formation. Astronomy and Astrophysics - A&A, 2021, 655 (2), pp.A84. ⟨10.1051/0004-6361/202140963⟩. ⟨hal-03799860⟩Link
2021Á. Kóspál, F. Cruz-Sáenz de Miera, J. White, P. Ábrahám, L. Chen, et al.. Massive Compact Disks around FU Orionis–type Young Eruptive Stars Revealed by ALMA. The Astrophysical Journal Supplement, 2021, 256 (2), pp.30. ⟨10.3847/1538-4365/ac0f09⟩. ⟨insu-03439571⟩Link
2021S. Suri, H. Beuther, C. Gieser, Á. Sánchez-Monge, J. M. Winters, et al.. Disk fragmentation in high-mass star formation. High-resolution observations towards AFGL 2591-VLA 3. Astronomy and Astrophysics - A&A, 2021, ⟨10.1051/0004-6361/202140963⟩. ⟨insu-03439583⟩Link
2021Gisela Ortiz-León, Karl Menten, Andreas Brunthaler, Timea Csengeri, James Urquhart, et al.. A global view on star formation: the GLOSTAR Galactic plane survey. Astronomy and Astrophysics - A&A, 2021, 651, pp.A87. ⟨10.1051/0004-6361/202140817⟩. ⟨insu-03439597⟩Link
2021N. Biver, D. Bockelée-Morvan, D. C Lis, D. Despois, R. Moreno, et al.. Molecular composition of short-period comets from millimetre-wave spectroscopy: 21P/Giacobini-Zinner, 38P/Stephan-Oterma, 41P/Tuttle-Giacobini-Kresák, and 64P/Swift-Gehrels. Astronomy and Astrophysics - A&A, 2021, 651, pp.A25. ⟨10.1051/0004-6361/202140765⟩. ⟨hal-03425697⟩Link
2021H. Nguyen, M. Rugel, K. Menten, A. Brunthaler, S. Dzib, et al.. A global view on star formation: The GLOSTAR Galactic plane survey. Astronomy and Astrophysics - A&A, 2021, 651, pp.A88. ⟨10.1051/0004-6361/202140802⟩. ⟨insu-03439601⟩Link
2021A. Brunthaler, K. Menten, S. Dzib, W. Cotton, F. Wyrowski, et al.. A global view on star formation: The GLOSTAR Galactic plane survey. Astronomy and Astrophysics - A&A, 2021, 651, pp.A85. ⟨10.1051/0004-6361/202039856⟩. ⟨insu-03439592⟩Link
2021Aina Palau, Qizhou Zhang, Josep Girart, Junhao Liu, Ramprasad Rao, et al.. Does the Magnetic Field Suppress Fragmentation in Massive Dense Cores?. The Astrophysical Journal, 2021, 912 (2), pp.159. ⟨10.3847/1538-4357/abee1e⟩. ⟨hal-03445978⟩Link
2021M. Wienen, F. Wyrowski, C. Walmsley, T. Csengeri, T. Pillai, et al.. ATLASGAL-selected massive clumps in the inner Galaxy. Astronomy and Astrophysics - A&A, 2021, 649, pp.A21. ⟨10.1051/0004-6361/201731208⟩. ⟨insu-03439608⟩Link
2021M. Beltrán, V. Rivilla, R. Cesaroni, L. Maud, D. Galli, et al.. Fragmentation in the massive G31.41+0.31 protocluster. Astronomy and Astrophysics - A&A, 2021, 648, pp.A100. ⟨10.1051/0004-6361/202040121⟩. ⟨insu-03439617⟩Link
2021C. Gieser, H. Beuther, D. Semenov, A. Ahmadi, S. Suri, et al.. Physical and chemical structure of high-mass star-forming regions. Astronomy and Astrophysics - A&A, 2021, 648, pp.A66. ⟨10.1051/0004-6361/202039670⟩. ⟨hal-03232031⟩Link
2021Hussein Yahia, Nicola Schneider, Sylvain Bontemps, Lars Bonne, Guillaume Attuel, et al.. Description of turbulent dynamics in the interstellar medium: Multifractal-microcanonical analysis: I. Application to Herschel observations of the Musca filament. Astronomy and Astrophysics - A&A, 2021, ⟨10.1051/0004-6361/202039874⟩. ⟨hal-03193056⟩Link
2021L. Moscadelli, H. Beuther, A. Ahmadi, C. Gieser, F. Massi, et al.. Multi-scale view of star formation in IRAS 21078+5211: from clump fragmentation to disk wind. Astronomy and Astrophysics - A&A, 2021, 647, pp.A114. ⟨10.1051/0004-6361/202039837⟩. ⟨insu-03439628⟩Link
2021A. Duarte-Cabral, D. Colombo, J Urquhart, A. Ginsburg, D. Russeil, et al.. The SEDIGISM survey: molecular clouds in the inner Galaxy. Monthly Notices of the Royal Astronomical Society, 2021, 500 (3), pp.3027-3049. ⟨10.1093/mnras/staa2480⟩. ⟨hal-03046472⟩Link
2021F. Schuller, P. André, Y. Shimajiri, Annie Zavagno, N. Peretto, et al.. VizieR Online Data Catalog: Probing the ISF in Orion A with ArTeMiS (Schuller+, 2021). VizieR Online Data Catalog, 2021, pp.J/A+A/651/A36. ⟨hal-03561795⟩Link
2021F. Schuller, J Urquhart, T. Csengeri, D. Colombo, A. Duarte-Cabral, et al.. The SEDIGISM survey: First Data Release and overview of the Galactic structure. Monthly Notices of the Royal Astronomical Society, 2021, 500 (3), pp.3064-3082. ⟨10.1093/mnras/staa2369⟩. ⟨hal-03046462⟩Link
2021Bernd Vollmer, Jonathan Braine, Barbara Mazzilli-Ciraulo, B. Schneider. Low star formation efficiency due to turbulent adiabatic compression in the Taffy bridge. Astronomy and Astrophysics - A&A, 2021, 647, pp.A138. ⟨10.1051/0004-6361/202037887⟩. ⟨hal-03185769⟩Link
2021Emeric E. Bron, Evelyne Roueff, Maryvonne Gerin, Jérôme Pety, Pierre Gratier, et al.. Tracers of the ionization fraction in dense and translucent gas: I. Automated exploitation of massive astrochemical model grids. Astronomy and Astrophysics - A&A, 2021, 645, pp.A28. ⟨10.1051/0004-6361/202038040⟩. ⟨hal-03017390⟩Link
2021Antoine Roueff, Maryvonne Gerin, Pierre Gratier, François Levrier, Jérôme Pety, et al.. C18O, 13CO, and 12CO abundances and excitation temperatures in the Orion B molecular cloud: Analysis of the achievable precision in modeling spectral lines within the approximation of the local thermodynamic equilibrium. Astronomy and Astrophysics - A&A, 2021, 645 (A26), ⟨10.1051/0004-6361/202037776⟩. ⟨hal-02570214v2⟩Link
2021F. Schuller, Ph. André, Y. Shimajiri, Annie Zavagno, N. Peretto, et al.. Probing the structure of a massive filament: ArTéMiS 350 and 450 μm mapping of the integral-shaped filament in Orion A. Astronomy and Astrophysics - A&A, 2021, 651, pp.A36. ⟨10.1051/0004-6361/202038259⟩. ⟨cea-03285690⟩Link
2021J Urquhart, C Figura, J. Cross, M Wells, T. Moore, et al.. SEDIGISM-ATLASGAL: dense gas fraction and star formation efficiency across the Galactic disc. Monthly Notices of the Royal Astronomical Society, 2021, 500 (3), pp.3050-3063. ⟨10.1093/mnras/staa2512⟩. ⟨hal-03046484⟩Link
2021N. Biver, D. Bockelée-Morvan, D. C. Lis, D. Despois, R. Moreno, et al.. Molecular composition of short-period comets from millimetre-wave spectroscopy: 21P/Giacobini-Zinner, 38P/Stephan-Oterma, 41P/Tuttle-Giacobini-Kresák, and 64P/Swift-Gehrels. Astronomy and Astrophysics - A&A, 2021, 651, pp.A25. ⟨10.1051/0004-6361/202140765⟩. ⟨hal-03285131⟩Link
2021Pierre Gratier, Jérôme Pety, Emeric Bron, Antoine Roueff, Jan H. Orkisz, et al.. Quantitative inference of the H2 column densities from 3 mm molecular emission: case study towards Orion B. Astronomy and Astrophysics - A&A, 2021, 645, pp.A27. ⟨10.1051/0004-6361/202037871⟩. ⟨hal-03017404v2⟩Link
2021V. Wakelam, P. Gratier, M. Ruaud, R. Le Gal, L. Majumdar, et al.. Chemical compositions of five Planck cold clumps. Astronomy and Astrophysics - A&A, 2021, 647, pp.A172. ⟨10.1051/0004-6361/202039367⟩. ⟨hal-03185772⟩Link
2021S. Pezzuto, M. Benedettini, J. Di Francesco, P. Palmeirim, S. Sadavoy, et al.. Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations. Astronomy and Astrophysics - A&A, 2021, 645, pp.A55. ⟨10.1051/0004-6361/201936534⟩. ⟨hal-03445984⟩Link
2020James Di Francesco, Jared Keown, Cassandra Fallscheer, Philippe André, Bilal Ladjelate, et al.. Herschel Gould Belt Survey Observations of Dense Cores in the Cepheus Flare Clouds. The Astrophysical Journal, 2020, 904 (2), pp.172. ⟨10.3847/1538-4357/abc016⟩. ⟨hal-03445941⟩Link
2020Damien Albert, Bobby K Antony, Yaye Awa Ba, Yuri L Babikov, Philippe Bollard, et al.. A Decade with VAMDC: Results and Ambitions. Atoms, 2020, 8 (4), pp.76. ⟨10.3390/atoms8040076⟩. ⟨hal-03030550⟩Link
2020A. Longobardi, A. Boselli, M. Fossati, J. A. Villa-Vélez, S. Bianchi, et al.. A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE): VII. Bridging the cluster-ICM-galaxy evolution at small scales. Astronomy and Astrophysics - A&A, 2020, 644, pp.A161. ⟨10.1051/0004-6361/202039020⟩. ⟨hal-03070769⟩Link
2020G. Sabatini, S. Bovino, A. Giannetti, F. Wyrowski, M. Órdenes, et al.. Survey of ortho-H 2 D + in high-mass star-forming regions. Astronomy and Astrophysics - A&A, 2020, 644, pp.A34. ⟨10.1051/0004-6361/202039010⟩. ⟨hal-03040674⟩Link
2020Ward Homan, Miguel Montargès, Bannawit Pimpanuwat, Anita Richards, Sofia Wallström, et al.. ATOMIUM: A high-resolution view on the highly asymmetric wind of the AGB star π 1 Gruis. Astronomy and Astrophysics - A&A, 2020, 644, pp.A61. ⟨10.1051/0004-6361/202039185⟩. ⟨hal-03190441⟩Link
2020A. Coutens, B. Commerçon, V. Wakelam. Chemical evolution during the formation of a protoplanetary disk. Astronomy and Astrophysics - A&A, 2020, 643, pp.A108. ⟨10.1051/0004-6361/202038437⟩. ⟨hal-03001912⟩Link
2020E. Fiorellino, D. Elia, Ph André, A. Men'Shchikov, S. Pezzuto, et al.. The census of dense cores in the Serpens region from the Herschel Gould Belt Survey. Monthly Notices of the Royal Astronomical Society: Letters, 2020, ⟨10.1093/mnras/staa3420⟩. ⟨hal-03019292⟩Link
2020Lars Bonne. The formation of dense gas in low- and high-mass star forming regions. Astrophysics [astro-ph]. Université de Bordeaux, 2020. English. ⟨NNT : 2020BORD0121⟩. ⟨tel-03121145⟩Link
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2015J. D., Adams, T. L., Herter, J. L., Hora, N. Schneider, R. M., Lau, et al.. SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment. The Astrophysical Journal, 2015, 814 (1), pp.id. 54. ⟨10.1088/0004-637X/814/1/54⟩. ⟨hal-01217944⟩Link
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2015F. Lelli, P. -A. Duc, E. Brinks, F. Bournaud, S. S. Mcgaugh, et al.. Gas dynamics in tidal dwarf galaxies: disc formation at z=0. Astronomy and Astrophysics - A&A, 2015, 584, pp.A113. ⟨10.1051/0004-6361/201526613⟩. ⟨hal-01202941⟩Link
2015A., Rivera-Ingraham, P. G., Martin, D., Polychroni, N. Schneider, F., Motte, et al.. Herschel Observations of the W3 GMC (II): Clues to the Formation of Clusters of High-Mass Stars. The Astrophysical Journal, 2015, 809 (1), pp.id. 81. ⟨10.1088/0004-637X/809/1/81⟩. ⟨hal-01174415⟩Link
2015Celia, Verdugo, Francoise Combes, Kalliopi, Dasyra, Phillipe, Salome, J. Braine. Ram Pressure Stripping in the Virgo Cluster. Astronomy and Astrophysics - A&A, 2015, 582, pp.id.A6. ⟨10.1051/0004-6361/201526551⟩. ⟨hal-01178408⟩Link
2015Hao, Chen, Yu, Gao, J. Braine, Qiusheng, Gu. Spatially-Resolved Dense Molecular Gas and Star Formation Rate in M51. The Astrophysical Journal, 2015, 810 (2), pp.id. 140. ⟨10.1088/0004-637X/810/2/140⟩. ⟨hal-01197442⟩Link
2015E., de Beck, W., Vlemmings, S., Muller, J. H., Black, E., O'Gorman, et al.. ALMA observations of TiO$_2$ around VY Canis Majoris. Astronomy and Astrophysics - A&A, 2015, 580, pp.A36. ⟨10.1051/0004-6361/201525990⟩. ⟨hal-01159884⟩Link
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2015N. Schneider, T. Csengeri, R. S. Klessen, Pascal Tremblin, V. Ossenkopf, et al.. Understanding star formation in molecular clouds. II. Signatures of gravitational collapse of IRDCs. Astronomy and Astrophysics - A&A, 2015, 578, pp.id.A29. ⟨10.1051/0004-6361/201424375⟩. ⟨hal-01092258⟩Link
2015N. Schneider, V., Ossenkopf, T., Csengeri, R. S., Klessen, C., Federrath, et al.. Understanding star formation in molecular clouds. I. Effects of line-of-sight contamination on the column density structure. Astronomy and Astrophysics - A&A, 2015, 575, pp.A79. ⟨10.1051/0004-6361/201423569⟩. ⟨hal-00958750⟩Link
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2015Sarah Fechtenbaum, Sylvain Bontemps, N. Schneider, T., Csengeri, A. Duarte-Cabral, et al.. First detection of CF+ towards a high-mass protostar. Astronomy and Astrophysics - A&A, 2015, 574, pp.id.L4. ⟨10.1051/0004-6361/201424718⟩. ⟨hal-01109640⟩Link
2015Catarina, Alves de Oliveira, N. Schneider, Bruno, Merín, Timo, Prusti, Álvaro, Ribas, et al.. Herschel view of the large-scale structure in the Chamaeleon dark clouds. 2015IAUGA.2252675A - IAU General Assembly, Meeting #29, #2252675 - held 4-8 January 2015 in Seattle, USA, Jan 2015, Seattle, United States. pp.52675. ⟨hal-01197438⟩Link
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2015Frederique, Motte, Sylvain Bontemps, Quang, Nguyen Luong. HOBYS and W43, two more steps towards a Galaxy-wide understanding of star formation. 2015IAUGA.2258331M - IAU General Assembly, Meeting #29, #2258331 - held 4-8 January 2015 in Seattle, USA, Jan 2015, Seattle, United States. pp.58331. ⟨hal-01197416⟩Link
2015Frederique, Motte, Sylvain Bontemps, Tracey, Hill. High mass star and cluster formation: new insights from Herschel. 2015IAUGA.2258385M - IAU General Assembly, Meeting #29, #2258385 - held 4-8 January 2015 in Seattle, USA, Jan 2015, Seattle, United States. pp.58385. ⟨hal-01197413⟩Link
2015Quang, Nguyen Luong, Frederique, Motte, Hans, Nguyen, N. Schneider, Fabien, Louvet. COnnecting LOcal to GLObal star formation via MIni-starburst. 2015IAUGA.2255299N - IAU General Assembly, Meeting #29, #2255299 - held 4-8 January 2015 in Seattle, USA, Jan 2015, Seattle, United States. pp.55299. ⟨hal-01197434⟩Link
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2015Sylvain Bontemps, N. Schneider, Frederique, Motte. Filaments, ridges and the origin of high-mass stars and clusters in Cygnus X. 2015IAUGA.2257007B - IAU General Assembly, Meeting #29, #2257007- held 4-8 January 2015 in Seattle, USA, Jan 2015, Seattle, United States. pp.57007. ⟨hal-01197408⟩Link
2015Joseph D., Adams, Terry, Herter, Ryan M., Lau, Joseph L., Hora, N. Schneider, et al.. The Warm Dust Component in the S106 Region. American Astronomical Society, AAS Meeting #225, #141.15, held 4-8 January 2015 at the Washington State Convention & Trade Center in Seattle, WA., Jan 2015, Seattle, United States. ⟨hal-01137427⟩Link
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2015N. Brouillet, D. Despois, X. -H. Lu, Alain Baudry, J. Cernicharo, et al.. Antifreeze in the hot core of Orion - First detection of ethylene glycol in Orion-KL. Astronomy and Astrophysics - A&A, 2015, 576, pp.id.A129. ⟨10.1051/0004-6361/201424588⟩. ⟨hal-01117920⟩Link
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2015N. Schneider, Sylvain Bontemps, P. Girichidis, T. Rayner, F. Motte, et al.. Detection of two power-law tails in the probability distribution functions of massive GMCs. Monthly Notices of the Royal Astronomical Society, 2015, 453, pp.41-45. ⟨10.1093/mnrasl/slv101⟩. ⟨hal-01197448⟩Link
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2015W. H. T., Vlemmings, S., Ramstedt, E., O'Gorman, E. M. L., Humphreys, M., Wittkowski, et al.. Resolving the stellar activity of the Mira AB binary with ALMA. Astronomy and Astrophysics Supplement Series, 2015, 577, pp.id.L4. ⟨10.1051/0004-6361/201526186⟩. ⟨hal-01136924⟩Link
2015N. Schneider, V., Ossenkopf, T., Csengeri, R., Klessen, C., Federrath, et al.. VizieR Online Data Catalog: SPIRE 250um maps of 4 molecular clouds (Schneider+, 2015). 2015, pp.50079. ⟨hal-01238837⟩Link
2015M., Wienen, F., Wyrowski, K. M., Menten, J. S., Urquhart, T., Csengeri, et al.. ATLASGAL - Kinematic distances and the dense gas mass distribution of the inner Galaxy. Astronomy and Astrophysics - A&A, 2015, 579, pp.id.A91. ⟨10.1051/0004-6361/201424802⟩. ⟨hal-01137212⟩Link
2014A. M. S. Richards, C. M. V. Impellizzeri, E. M. Humphreys, C. Vlahakis, W. Vlemmings, et al.. ALMA reveals VYCMa's sub-mm maser and dust distribution. Revolution in Astronomy with ALMA: The Third Year. Proceedings of a Conference held at the Tokyo International Forum, Tokyo, Japan 8-11 December 2014. Edited by Daisuke Iono, Ken-ichi Tatematsu, Alwyn Wootten, and Leonardo Testi. ASP Conference Series Vol. 499. San Francisco: Astronomical Society of the Pacific, 2015, p.337, Dec 2014, Tokyo, Japan. ⟨hal-01067310⟩Link
2014A. Coutens, C. Vastel, U. Hincelin, E. Herbst, D. Lis, et al.. Water deuterium fractionation in the high-mass star-forming region G34.26+0.15 based on Herschel/HIFI data. Monthly Notices of the Royal Astronomical Society, 2014, 445 (2), pp.1299-1313. ⟨10.1093/mnras/stu1816⟩. ⟨hal-02558307⟩Link
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2014Shipman R. F.,, van Der Tak F. F. S.,, Wyrowski F.,, Fabrice Herpin, Frieswijk W.,. The physical conditions in IRDC clumps from Herschel/HIFI observations of H2O. Astronomy and Astrophysics - A&A, 2014, 570, pp.51. ⟨10.1051/0004-6361/201423912⟩. ⟨hal-01061817⟩Link
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2014Shipman R.,, van Der Tak F. F. S.,, Wyrowski F.,, Fabrice Herpin, Frieswijk W.,. VizieR Online Data Catalog: 4 IRDC clump C17O, H2O, and N2H spectra (Shipman+, 2014). 2014, pp.09051. ⟨hal-01078153⟩Link
2014J. S. Urquhart, T. Csengeri, F. Wyrowski, F. Schuller, Sylvain Bontemps, et al.. VizieR Online Data Catalog: ATLASGAL Compact Source Catalog: 280Link
2014A. Duarte-Cabral, Sylvain Bontemps, F. Motte, M. Hennemann, N. Schneider, et al.. VizieR Online Data Catalog: Cygnus-X CO and SiO outflows datacubes (Duarte-Cabral+, 2014). 2014, pp.09001. ⟨hal-01078801⟩Link
2014R. P. J. Tilanus, T. P. Krichbaum, J. A. Zensus, Alain Baudry, W. Vlemmings, et al.. Future mmVLBI Research with ALMA: A European vision. 2014. ⟨hal-01011134⟩Link
2014C. Favre, Miguel, Carvajal, David, Field, Edwin, Bergin, Justin, Neill, et al.. 13C-METHYL Formate in Orion-Kl Alma Observations and Spectroscopic Characterization. 2014isms.confETF06F - 69th International Symposium on Molecular Spectroscopy: June 16-20, 2014 at The University of Illinois at Urbana-Champaign. Talk TF06, Jun 2014, Urbana-Champaign, United States. ⟨hal-01136345⟩Link
2014N. Schneider, T. Csengeri, R. S. Klessen, Pascal Tremblin, V. Ossenkopf, et al.. On the similarity of IR-bright and IR-dark molecular clouds. 2014. ⟨hal-01011115⟩Link
2014T. Csengeri, J. S. Urquhart, F. Schuller, F. Motte, Sylvain Bontemps, et al.. VizieR Online Data Catalog: ATLASGAL. Dust condensations in Galactic plane (Csengeri+, 2014). 2014, pp.59075. ⟨hal-01071906⟩Link
2014T. Cavalié, R. Moreno, E. Lellouch, P. Hartogh, O. Venot, et al.. The first submillimeter observation of CO in the stratosphere of Uranus. Astronomy and Astrophysics - A&A, 2014, 562, pp.33. ⟨10.1051/0004-6361/201322297⟩. ⟨hal-00904019⟩Link
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2014T. Cavalié, O. Venot, Franck Selsis, F. Hersant, P. Hartogh. The Deep O/H Ratio in Uranus and Neptune from CO Spectroscopy and Thermochemical Modeling. the Study of the Ice Giant Planets, 2014, Laurel, United States. pp.2011. ⟨hal-01059927⟩Link
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2014S. I. Sadavoy, J. Di Francesco, Ph. Andre, S. Pezzuto, J. -P. Bernard, et al.. Class 0 Protostars in the Perseus Molecular Cloud: A Correlation Between the Youngest Protostars and the Dense Gas Distribution. The Astrophysical journal letters, 2014, 787 (2), pp.L18. ⟨10.1088/2041-8205/787/2/L18⟩. ⟨hal-00987362⟩Link
2014A. Lèbre, M. Aurière, N. Fabas, D. Gillet, Fabrice Herpin, et al.. Search for Surface Magnetic Fields in Mira Stars. First Detection in chi Cyg. Astronomy and Astrophysics - A&A, 2014, 561, pp.id.A85. ⟨10.1051/0004-6361/201322826⟩. ⟨hal-00874484⟩Link
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