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Discovery of gas accretion onto stars in 13 Myr old H and X persei

Author
CURRIE, Thayne1 ; KENYON, Scott J1 ; BALOG, Zoltan2 3 ; BRAGG, Ann4 ; TOKARZ, Susan1
[1] Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02140, United States
[2] Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, United States
[3] On leave from the Department of Optics and Quantum Electronics, Uni versity of Szeged, 6720 Szeged, Hungary
[4] Department of Physics, Bowling Green State University, Bowling Green, OH 43403, United States
Source

The Astrophysical journal. 2007, Vol 669, Num 1 ; L33-L36 ; 2 ; ref : 1/4 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
accretion, accretion disks open clusters and associations: individual (NGC 869, NGC 884) planetary systems: protoplanetary disks
Keyword (fr)
Accrétion stellaire Amas ouvert Amas stellaire Disque accrétion Nébuleuse proto planétaire Système planétaire
Keyword (en)
Star accretion Open clusters Star clusters Accretion disks Proto planetary nebula 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
19193974

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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