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HN Peg B : A TEST OF MODELS OF THE L TO T DWARF TRANSITION

Author
LEGGETT, S. K1 ; SAUMON, D2 ; ALBERT, Loic3 ; GUSHING, Michael C4 ; LIU, Michael C4 ; LUHMAN, K. L5 ; MARLEY, M. S6 ; KIRKPATRICK, J. Davy7 ; ROELLIG, Thomas L6 ; ALLERS, K. N4
[1] Gemini Observatory, Northem Operations Center, 670 North A'ohoku Place, Hilo, HI 96720, United States
[2] Los Alamos National Laboratory, P.O. Box 1663, MS F663, Los Alamos, NM 87545, United States
[3] Canada-France-Hawaii Telescope Corporation, 65-1238 Mamalahoa Highway, Kamuela, HI 96743, United States
[4] Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, United States
[5] Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16802, United States
[6] NASA Ames Research Center, Mail Stop 245-3, Moffett Field, CA 94035, United States
[7] IPAC, California Institute of Technology, Mail Code 100-22, 770 South Wilson Avenue, Pasadena, CA 91125, United States
Source

The Astrophysical journal. 2008, Vol 682, Num 2, pp 1256-1263, 8 p ; 1 ; 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
HN Peg B- stars: low-mass HN Peg binaries: visual-stars: individual 2MASS J21442847+1446077 brown dwarfs
Keyword (fr)
Binaire visuelle Etoile B Etoile faible masse Modèle Naine brune
Keyword (en)
Visual binary stars B stars Low-mass stars Models Brown dwarf stars
Keyword (es)
Modelo
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20547435

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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