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Integrated-light VRI imaging photometry of globular clusters in the Magellanic Clouds

Author
GOUDFROOIJ, Paul1 ; GILMORE, Diane1 ; KISSLER-PATIG, Markus2 ; MARASTON, Claudia3
[1] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States
[2] European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany
[3] University of Oxford, Astrophysics, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, United Kingdom
Source

Monthly Notices of the Royal Astronomical Society. 2006, Vol 369, Num 2, pp 697-704, 8 p ; ref : 60 ref

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Blackwell Science, Oxford
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
Magellanic Clouds galaxies: evolution galaxies: star clusters techniques: photometric
Keyword (fr)
Age Amas galaxies Amas globulaire Amas stellaire Branche géante asymptotique Couleur Etoile géante Etoile rouge Géante rouge Luminosité Modèle stellaire Métallicité Nuages Magellan Photométrie Population stellaire Evolution galaxies
Keyword (en)
Age Galaxy clusters Globular clusters Star clusters Asymptotic giant branch Color Giant stars Red stars Red giant stars Luminosity Star models Metallicity Magellanic Clouds Photometry Stellar population Galaxy evolution
Keyword (es)
Edad Rama gigante asintótica Metalicidad Población estelar Evolución galaxias
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
17838867

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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