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A binary model for the UV-upturn of elliptical galaxies

Author
HAN, Z1 ; PODSIADLOWSKI, Ph2 ; LYNAS-GRAY, A. E2
[1] National Astronomical Observatories/Yunnan Observatoly, The Chinese Academy of Sciences, Kunming 650011, China
[2] Department of Physics, University of Oxford, Keble Road, Oxford 0X1 3RH, United Kingdom
Source

Monthly Notices of the Royal Astronomical Society. 2007, Vol 380, Num 3, pp 1098-1118, 21 p ; ref : 1 p.1/2

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
binaries: close galaxies: elliptical and lenticular, cD galaxies: starburst subdwarfs ultraviolet: galaxies
Keyword (fr)
Age Binaire serrée Combustion hélium Combustion stellaire Diagramme 2 couleurs Déplacement vers le rouge Etoile chaude Etoile hélium Etoile jeune Excès UV Galaxies elliptiques Galaxies lenticulaires Galaxies à flambée Modèle Métallicité Sous naine Spectre UV
Keyword (en)
Age Close binary stars Helium burning Star burning Two color diagram Red shift Hot star Helium stars Young stars Ultraviolet excess Elliptical galaxies Lenticular galaxies Starburst galaxies Models Metallicity Subdwarf Ultraviolet spectra
Keyword (es)
Edad Diagrama 2 colores Estrella caliente Exceso UV Galaxias llamarada estelar Modelo Metalicidad Subenana
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
19067118

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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