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Kinematic evidence for an old stellar halo in the Large Magellanic Cloud

Author
MINNITI, Dante1 ; BORISSOVA, Jura1 ; REJKUBA, Marina2 ; ALVES, David R3 ; COOK, Kem H4 ; FREEMAN, Kenneth C5
[1] Department of Astronomy, Pontificia Universidad Católica, Aveñida Vicuña Mackenna 4860, Casilla 306, Santiago 22, Chile
[2] European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany
[3] Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027, United States
[4] Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, Livermore, CA 94550, United States
[5] Research School of Astronomy and Astrophysics, Australian National University, Mount Stromlo Observatory, Canberra, ACT, Australia
Source

Science (Washington, D.C.). 2003, Vol 301, Num 5639, pp 1508-1510, 3 p ; ref : 36 ref

CODEN
SCIEAS
ISSN
0036-8075
Scientific domain
Multidisciplinary
Publisher
American Association for the Advancement of Science, Washington, DC
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Cinématique stellaire Dispersion vitesse Etoile pauvre en métal Etoile type RR Lyrae Grand Nuage Magellan Halo galactique Spectre optique Traceur
Keyword (en)
Stellar kinematics Velocity dispersion Metal-poor stars RR Lyrae stars Large Magellanic Cloud Galactic halos Optical spectrum Tracers
Keyword (es)
Cinematica estelar Dispersión velocidad Espectro óptico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C20 Normal stars (by class): general or individual / 001E03C20T Population ii stars (horizontal branch, metal poor, etc.)

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D56 Local group. Magellanic clouds / 001E03D56S Magellanic clouds and other irregular galaxies

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
15163961

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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