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F. Combes

As seen in: Nature, Astronomy and Astrophysics (A&A)
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Articles by F. Combes

Evidence for a sub-Jovian planet in the young TWA 7 disk  - Nature

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By A.-M. Lagrange, M. C. Malin, C. Perrot, L. Matrà, F. Combes, D. Rouan, J. Milli, O. Flasseur, J. Olofsson, A. Lloris Bayo, Q. Kral, A. J. Carter, P. Delorme, P. Rubini, J. Mazoyer, T. Bodrito
| Nature Verified
Abstract Planets are thought to form from dust and gas in protoplanetary disks, with debris disks being the remnants of planet formation. Aged a few million up to a few billion years, debris disks have lost their primordial gas, and their dust is produced by steady-state collisions between larger, rocky bodies1,2.
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Environmental processing in cluster core galaxies at $z$ = 1.7

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By G. Castignani, F. Combes, Collège de France, P. Salomé
| hal.science
Environmental processing in cluster core galaxies at $z$ = 1.7 Mots clés galaxies: clusters: individual: SpARCS104922.6+564032.5 galaxies: clusters: general galaxies: star formation galaxies: evolution galaxies: active galaxies: ISM Origine : Fichiers éditeurs autorisés sur une archive ouverte
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Molecular gas in distant brightest cluster galaxies

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By G. Castignani, F. Combes, Collège de France, P. Salomé
| hal.science
Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2020 Molecular gas in distant brightest cluster galaxies Mots clés galaxies: clusters: general galaxies: star formation galaxies: evolution galaxies: active molecular data Origine : Fichiers éditeurs autorisés sur une archive ouverte hal-02467211 , version 1 (27-05-2024) G. Castignani, F. Combes, P. Salomé, J. Freundlich. Molecular gas in distant brightest cluster galaxies. Astronomy and Astrophysics - A&A, 2020, 635, pp.A32.
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Molecular gas and star formation activity in luminous infrared galaxies in clusters at intermediate redshifts

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By G. Castignani, P. Jablonka, F. Combes, Collège de France
| hal.science
Molecular gas and star formation activity in luminous infrared galaxies in clusters at intermediate redshifts Mots clés galaxies: clusters: general galaxies: star formation molecular data submillimeter: galaxies Origine : Fichiers éditeurs autorisés sur une archive ouverte
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Does absorption against AGN reveal supermassive black hole accretion?

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By Tom Rose, F. Combes, Collège de France, B.R. Mcnamara
| hal.science
Does absorption against AGN reveal supermassive black hole accretion? Mots clés ISM: molecules galaxies: ISM quasars: absorption lines Origine : Fichiers éditeurs autorisés sur une archive ouverte
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