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A SUBSTELLAR COMMON PROPER-MOTION COMPANION TO THE PLEIAD H II 1348

Author
GEISSLER, Kerstin1 ; METCHEV, Stanimir A1 ; PHAM, Alfonse2 ; LARKIN, James E3 ; MCELWAIN, Michael4 ; HILLENBRAND, Lynne A5
[1] Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800, United States
[2] Center for Exploration of Energy and Matter, Indiana University, Bloomington, IN 47408-1398, United States
[3] Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1562, United States
[4] Astrophysics Science Division, NASA Goddard Space Flight Center, Laboratory for Exoplanets and Stellar Astrophysics, Greenbelt, MD 20771, United States
[5] Department of Physics, Mathematics, and Astronomy, MC 105-24, California Institute of Technology, Pasadena, CA 91125, United States
Source

The Astrophysical journal. 2012, Vol 746, Num 1 ; 44.1-44.7 ; 1 ; ref : 1/2 p

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
binaries: visual brown dwarfs instrumentation: adaptive optics stars: individual (Cl Melotte 22 1348) stars: low-mass
Keyword (fr)
Age Amas ouvert Amas stellaire Astrométrie Binaire spectroscopique Binaire visuelle Etoile faible masse Modèle Mouvement propre Naine brune Optique adaptative Pléiades Source ponctuelle Spectrométrie Système hiérarchisé Type spectral
Keyword (en)
Age Open clusters Star clusters Astrometry Spectroscopic binary stars Visual binary stars Low-mass stars Models Proper motion Brown dwarf stars Adaptive optics Pleiades Point sources Spectroscopy Hierarchical systems Spectral type
Keyword (es)
Edad Modelo Tipo espectral
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
25489548

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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