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Cold disks : Spitzer spectroscopy of disks around young stars with large gaps

Author
BROWN, J. M1 ; BLAKE, G. A2 ; PONTOPPIDAN, K. M2 ; VAN DISHOECK, E. F4 ; DULLEMOND, C. P3 ; MERIN, B4 ; AUGEREAU, J. C4 5 ; BOOGERT, A. C. A6 ; EVANS, N. J7 ; GEERS, V. C4 ; LAHUIS, F4 8 ; KESSLER-SILACCI, J. E7
[1] Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, United States
[2] Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, United States
[3] Max-Planck-institut fur Astrophysik, 69117 Heidelberg, Germany
[4] Leiden Observatory, Leiden University, 2300 RA Leiden, Netherlands
[5] Laboratoire d'Astrophysique de l'Observatoire de Grenoble, 38041 Grenoble, France
[6] IPAC, California Institute of Technology, Pasadena, CA 91125, United States
[7] Department of Astronomy, University of Texas, Austin, TX 78712-0259, United States
[8] SRON National Institute for Space Research, 9700 AV Groningen, Netherlands
Source

The Astrophysical journal. 2007, Vol 664, Num 2 ; L107-L110 ; 2 ; ref : 1/2 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
planetary systems: protoplanetary disks-stars: pre-main-sequence
Keyword (fr)
Etoile jeune Etoile pré séquence principale Nébuleuse proto planétaire Spectrométrie Système planétaire
Keyword (en)
Young stars Pre-main-sequence stars Proto planetary nebula Spectroscopy Planetary system
Keyword (es)
Nebulosa proto planetaria Sistema planetario
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18972381

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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