The SDSS-GALEX viewpoint of the truncated red sequence in field environments at z ∼ 0
- Author
- HAINES, C. P1 2 ; GARGIULO, A1 3 ; MERLUZZI, P1
[1] INAF -Osservatorio Astronomico di Capodimonte, via Moiariello 16, 80131 Napoli, Italy
[2] School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, United Kingdom
[3] Department of Physics, Università Federico II, Napoli, Italy - Source
Monthly Notices of the Royal Astronomical Society. 2008, Vol 385, Num 3, pp 1201-1210, 10 p ; ref : 3/4 p
- 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
- galaxies: clusters: general galaxies: evolution galaxies: luminosity function, mass function galaxies: stellar content
- Keyword (fr)
- Amas galaxies Contenu stellaire Couleur Diagramme magnitude couleur Déplacement vers le rouge Etude ciel Evolution galaxies Fonction luminosité Fonction masse Formation stellaire Galaxies Masse stellaire Photométrie Satellite GALEX
- Keyword (en)
- Galaxy clusters Stellar content Color Color-magnitude diagrams Red shift Sky surveys Galaxy evolution Luminosity function Mass function Star formation Galaxies Stellar mass Photometry GALEX satellite
- Keyword (es)
- Contenido estelar Evolución galaxias Función masa Satélite GALEX
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20235355
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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DOI
10.1111/j.1365-2966.2008.12954.x 
https://dx.doi.org/10.1111/j.1365-2966.2008.12954.x
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