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THE TEXES SURVEY FOR H2 EMISSION FROM PROTOPLANETARY DISKS

Author
BITNER, Martin A1 ; RICHTER, Matthew J2 ; NAJITA, Joan R7 ; CURRIE, Thayne8 ; LACY, John H1 ; HERCZEG, Gregory J3 ; GREATHOUSE, Thomas K4 ; JAFFE, Daniel T1 ; SALYK, Colette5 ; BLAKE, Geoffrey A5 ; HOLLENBACH, David J6 ; DOPPMANN, Greg W7
[1] Department of Astronomy, University of Texas at Austin, Austin, TX 78712, United States
[2] Physics Department, University of California at Davis, Davis, CA 95616, United States
[3] California Institute of Technology, Pasadena, CA 91125, United States
[4] Southwest Research Institute, San Antonio, TX 78209, United States
[5] Division of Geological and Planetary Sciences, California Institute of Technology, MS 150-21, Pasadena, CA 91125, United States
[6] NASA Ames Research Center, Moffett Field, CA 94035, United States
[7] National Optical Astronomy Observatory, Tucson, AZ 85719, United States
[8] Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, United States
Source

The Astrophysical journal. 2008, Vol 688, Num 2, pp 1326-1344, 19 p ; 1 ; ref : 1 p.1/4

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
IOP, Bristol
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
circumstellar matter infrared: stars planetary systems: protoplanetary disks stars: individual (AB Aur, DoAr 21, Elias 29, GSS 30 IRS 1, GV Tau N, HL Tau) stars: pre-main-sequence
Keyword (fr)
Etoile IR Matière circumstellaire Nébuleuse proto planétaire Système planétaire
Keyword (en)
Infrared star Circumstellar matter Proto planetary nebula Planetary system
Keyword (es)
Estrella IR 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
20905223

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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