FEMIS – Formation d’etoiles et Milieu InterStellaire

La formation des étoiles est le processus initiateur du cycle de la matière des galaxies et de son enrichissement en éléments lourds et est à l’origine de la formation des systèmes planétaires. Alors que le principe de la formation stellaire est simple (effondrement gravitationnel d’un nuage interstellaire), le détail du processus est mal compris, surtout pour les étoiles les plus massives.

L’équipe de Formation d'étoiles et Milieu Interstellaire du LAB s’intéresse aux questions liées aux processus physiques de la formation ; structuration, formation des nuages moléculaires et recherche de protoétoiles massives ; influence du champ magnétique ; et à l’astrochimie et recherche de molécules complexes vers les protoétoiles massives. En étendant nos études aux galaxies proches, nous abordons aussi l’universalité du processus pour différents environnements et pour tenter de contraindre certaines propriétés de la formation stellaire au cours des âges cosmiques.

 

Structuration du milieu interstellaire vers la formation des étoiles

Depuis quelques années la formation des étoiles de faible masse dans les nuages moléculaires proches connaît un changement de paradigme.

Au lieu d’un scénario dit “gravo-turbulent” qui proposait l’apparition aléatoire de pics de densité suffisamment importants pour entraîner un effondrement, un scénario plus dynamique basé sur la formation préalable de filaments denses se dessine. L’équipe cherche actuellement à découvrir précisément l’origine de ces filaments grâce à des nouvelles méthodes statistiques d’analyse en collaboration avec l’équipe GeoStat de l’INRIA Bordeaux, et à des observations de raies de refroidissement avec SOFIA (avion stratosphérique NASA-DLR) en collaboration avec l’Université de Cologne en Allemagne (projet ANR-DFG GENESIS). L’équipe est aussi impliquée dans la préparation du grand projet ESA-JAXA de télescope spatial SPICA (2,5m refroidi) qui permettra de détecter les raies de refroidissement les plus faibles liées à la structuration du milieu interstellaire.

L’équipe est aussi impliquée dans la préparation du grand projet ESA-JAXA de télescope spatial SPICA (2,5m refroidi) qui permettra de détecter les raies de refroidissement les plus faibles liées à la structuration du milieu interstellaire.

 

Origine et formation des étoiles massives

Le mécanisme de formation des étoiles massives n’est pas bien compris dans les scénarios de formation stellaire. Ces étoiles ont des masses très supérieures aux masses de Jeans (masse maximum limite pour l’effondrement gravitationnel) typiques du milieu interstellaire. L’équipe de formation stellaire participe à plusieurs projets ALMA (projets SPARKS et W43-HERO) cherchant à comprendre dans quels environnements et conditions les masses de Jeans peuvent être comparables aux masses de ces étoiles massives. Répondre à cette question permettrait peut être d’expliquer l’origine de la limite supérieure de masse des étoiles (environ 100 à 150 Msolaire).

 

Astrochimie des protoétoiles massives

L’astrochimie est un moyen de contraindre les processus à l’œuvre pendant la formation des étoiles et d’évaluer la possibilité d’une origine « interstellaire » des molécules dites complexes dont certaines sont pré-biotiques. L’équipe s’intéresse à l’origine et l’évolution des coeurs chauds (au dessus de 100 K) qui entourent les protoétoiles massives et qui contiennent de grandes quantités de molécules complexes. L’équipe traque ainsi les molécules complexes rares vers Orion BN/KL, l’une des deux cibles de référence pour ces travaux (SgrB2 étant la deuxième). Nous suivons aussi l’évolution astrochimique des protoétoiles massives pendant la formation des cœurs chauds pour tenter d’identifier les processus dominants de formation des molécules complexes. Ces travaux sont basés sur des relevés spectroscopiques, certains non biaisés, avec ALMA, NOEMA et le 30m de l’IRAM.

 

Evolution stellaire et champ magnétique

A l'autre extrémité de l'évolution stellaire les étoiles quittent la séquence principale lorsque les réactions de combustion nucléaire interne cessent. L'évolution stellaire est alors dominée par des phénomènes de perte de masse conduisant à l'enrichissement du milieu interstellaire environnant. ALMA, APEX et le 30m de IRAM sont utilisés pour sonder la chimie, la cinématique et la perte de masse des enveloppes circumstellaires de ces étoiles.

Le champ magnétique joue un rôle décisif à de nombreux stades de l’évolution stellaire, de la formation à la fin de vie des étoiles. L’équipe travaille aussi à la caractérisation du champ magnétique dans ces stades avancés de l’évolution stellaire avec le télescope de IRAM-30m et son instrument Xpol. La polarimétrie avec ALMA, et dans un avenir plus lointain avec l’instrument SAFARI-pol sur SPICA, ouvre des perspectives importantes pour les milieux protostellaire et interstellaire où une sensibilité et une résolution spatiale plus grandes sont indispensables.

 

La diversité et l’origine des évènements de formation stellaire dans le groupe local

Le groupe des galaxies proches, dit groupe local, offre une diversité importante de conditions galactiques à exploiter pour tester l’universalité du processus de structuration des nuages moléculaires et de formation des étoiles. L’équipe de formation stellaire du LAB s’intéresse à la relation entre la quantité de gaz dense et le taux de formation d’étoiles dans le groupe local, ainsi qu’aux propriétés des populations de nuages moléculaires, plus particulièrement dans la galaxie spirale M33 (projet HerM33es).

 

Membres actuels
Fabrice Herpin

Astronome CNAP

Responsable thématique

  • Formation des étoiles massives
  • Évolution stellaire
  • Spectroscopie radio et IR (IRAM, Herschel, ALMA)
  • Modélisation (RATRAN, LIME)
  • Instrumentation (Herschel, SPICA)

Page personnelle

Fabrice Herpin

Alain Baudry

Astronome CE, Prof. Emérite

• Milieu Interstellaire et circumstellaire

• Étoiles en formation et évoluées

• Interférométrie mm et submm

• Design Corrélateur et Back-End ALMA

Alain Baudry

Sylvain Bontemps

Directeur de Recherche CNRS

• Formation des étoiles massives

• Phases protostellaires

• Structuration des nuages moléculaires

• Interférométrie millimétrique (NOEMA et ALMA)

• Grandes cartographies Herschel, ATLASGAL

Page personnelle

Sylvain Bontemps

Jonathan Braine

Astronome (CNAP)

• Milieu interstellaire des galaxies proches

• Groupe local

• Interférométrie millimétrique

 

Jonathan Braine

Nathalie Brouillet

Astronome adjointe (CNAP)

• Milieu interstellaire

• Etude des molécules complexes

• Interférométrie millimétrique

Nathalie Brouillet

Timea Csengeri

Chargée de recherche (CNRS)

 • Relevées galactiques
 • Formation des étoiles massives
 • Interférométrie mm et submm
 • Spectroscopie dans la THz

Timea Csengeri

Pierre Gratier

Astronome adjoint • Milieu interstellaire • Galaxies du Groupe Local • Observations radio-millimétriques • Astrostatistique

Pierre Gratier

Thierry Jacq

Astronome adjoint

Formation des étoiles massives

Thierry Jacq

David Smith

Directeur de Recherche CNRS
  • Pulsars en rayon gamma, avec le Large Area Telescope (LAT) sur Fermi.
  • Ephemerides radio de rotation de pulsars.
  • Phénomènes cosmiques de haute énergie.

David Smith

Valentine Wakelam

Directrice de recherche CNRS

• Modélisation chimique

• Nuages denses, protoétoiles, disques protoplanétaires

Page personnelle

Valentine Wakelam

Maxime Valeille-Manet

Doctorant

  • Astrochimie des coeurs préstellaires massifs et de masse intermédiaire
  • Scénario de formation d'étoiles massives

Maxime Valeille-Manet

Louise Marinho

Doctorante

  • Etoiles évoluées

Louise Marinho

Aimie Clément

Doctorante

  • interaction rayons cosmiques milieu interstellaire 
  • résidus de supernovae
  • collaboration avec le LP2i

Aimie Clément

Nina Kessler

Doctorante

  • machine learning
  • milieu interstellaire et formation d'étoiles

Nina Kessler

Anciens membres
Alizée Duthu

Doctorante

• Champ magnétique étoiles évoluées

• Radio-astronomie

Alizée Duthu

Jordan Molet

Doctorant

• Recherche de molécules complexes

• Interférométrie millimétrique (ALMA)

Jordan Molet

Arabindo Roy

Postdoctorant

• Formation stellaire galactique

• Rôle des filaments dans la formation stellaire

• Milieu interstellaire

• Evolution de la matière interstellaire

Arabindo Roy

Mélisse BONFAND

Postdoc

  • Formation d'étoiles massives
  • Etude des molécules complexes
  • interferoétrie mm & submm (ALAMA)
  • Modélisation chimique

Mélisse BONFAND

Sami DIB

Postdoc
  • Modèles théorique/numérique
  • Fonction initiale de masse stellaire
  • Loi d'échelle de formation stellaire
  • Structure des  nuages de molécules

Page personnelle

Sami DIB

Lars Bonne

Etudiant en thèse

  • Formation des structures denses moleculaires
  •  Formation des etoiles massives
  •  Recherche de chocs a basse vitesse
  •  Astrochimie des coeurs pre-stellaires massifs

Lars Bonne

Didier Despois

Chargé de Recherche CNRS

• Molécules complexes et prébiotiques dans le milieu interstellaire

• Orion KL

• Lien avec les comètes

• Confusion spectrale

• Exobiologie

Didier Despois

Angèle Taillard

Doctorante

  • Phases précoces de la formation d'étoiles
  • Astrochimie
  • Observations mm et submm

Angèle Taillard

Karlis Dzenis

Doctorant

  • Etoiles évoluées
  • Astrophysique de laboratoire

Karlis Dzenis

Axe 1 : La formation et l’astrochimie des protoétoiles massives
Pour comprendre la composition moléculaire des enveloppes des protoétoiles massives, l’équipe est impliquée dans les projets millimétriques interférométriques principalement avec ALMA et NOEMA pour explorer la composition moléculaire des enveloppes massives à une résolution angulaire de ~1000-2000 u.a. Avec ALMA, NOEMA et sans doute avec SKA, une recherche systématique des molécules complexes (COMs) dans les régions de formation stellaire sera menée, notamment afin de contraindre leur origine, en lien avec la chimie des grains et/ou les chocs d’accrétion. Le projet Chaire Junior d’IdEX de l’UB, C-ORIGINS, a ainsi pour but de se concentrer sur la distribution et la diversité des COMs vers les protoétoiles massives. L'équipe est aussi fortement impliquée dans le Large Programme ALMA-IMF qui a pour but de recenser la population des protoétoiles dans un échantillon de proto-amas Galactiques, d’étudier l’évolution de la CMF et de comprendre l’origine de l’IMF. Des travaux complémentaires vers Orion BN-KL, ainsi que des études dans les nuages de Magellan seront menés.  
Un effort particulier est prévu pour participer au développement de méthodes automatiques d’extraction d’information des relevés spectraux larges ou non biaisés vers les proto-étoiles. Nous travaillerons également sur la modélisation 2D et 3D (raies et continuum) 

Axe 2 : La formation et l’astrochimie du milieu interstellaire 
La problématique de la formation des étoiles se tourne de plus en plus vers la compréhension de la formation des structures denses (filaments, coeurs denses, ridges massifs, coeurs denses massifs, “hubs”) qui se fragmentent en proto-étoiles. La formation de ces structures denses peut se relier aux scenarii de formation de complexes moléculaires à partir du gaz atomique et à l'équilibre global du milieu interstellaire (MIS) froid. C’est pendant la formation de ces nuages et structures denses que les conditions initiales de l’astrochimie se mettent en place. Le MIS diffus d’où émergent les structures denses est sous des influences diverses mal comprises : rayonnement UV, rayons cosmiques, champ magnétique, turbulence et dissipation, chocs … Nous devons aussi étudier les propriétés des nuages moléculaires dans des environnement divers en comparant des objets plus lointains aux objets plus proches donc mieux résolus. 

Axe 3 : Les étoiles évoluées et l’enrichissement interstellaire
Nous poursuivrons notre étude multi-instruments dans le cadre de l’ANR PEPPER et du LP ALMA-ATOMIUM afin d’obtenir une vue d’ensemble des processus physiques (notamment le champ magnétique) à l’œuvre des couches sub-photosphériques jusqu’à l’environnement circumstellaire. Notre but est de mieux comprendre la dynamique et la chimie de la phase gazeuse, la formation de poussière dans les vents et donc les phénomènes de perte de masse, et par conséquent l’enrichissement interstellaire. En lien avec ces projets, l’ANR WaterStars (collaboration LAB-ISM-IPAG) vise à étudier l’excitation ro-vibrationnelle de l’eau dans les étoiles évoluées (notamment pour les émissions maser). Il s’agit d’obtenir de nouvelles données de collision (sections efficaces ro-vibrationnelles et taux) au travers de nouveaux calculs et de nouvelles expériences, puis de les exploiter dans un modèle avancé de transfert radiatif de l’eau.
Une partie des recherches sur les étoiles évoluées concernera les étoiles massives qui ont évolué vers le stade du pulsar (à partir d’observations avec le Fermi LAT, Nançay, MeerKAT et, à terme, SKA) afin de mieux comprendre leur physique, notamment en exploitant les nombreuses détections de pulsars gamma, permettant ainsi de mieux estimer leur contribution à l’émission diffuse Gamma, ou de déterminer les mécanismes à l’origine des rayons cosmiques de haute énergie dans les nébuleuses de vent de pulsar.


Année Publication Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
2022N. Hambly, R. Andrae, F. de Angeli, M. Antonio, F. Arenou, et al.. Gaia DR3 documentation Chapter 20: Datamodel description. 2022. ⟨hal-03969804⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
2021Hussein Yahia, Nicola Schneider, Sylvain Bontemps, Lars Bonne, Guillaume Attuel, et al.. Description of turbulent dynamics in the interstellar medium: Multifractal-microcanonical analysis. Astronomy and Astrophysics - A&A, 2021, ⟨10.1051/0004-6361/202039874⟩. ⟨hal-03193056⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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⟩Lien
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. Astronomy and Astrophysics - A&A, 2021, 645, pp.A26. ⟨10.1051/0004-6361/202037776⟩. ⟨hal-02570214v2⟩Lien
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⟩Lien
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⟩Lien
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