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A close look at the Centaurus A group of galaxies IV. Recent star formation histories of late-type dwarfs around CenA

Author
CRNOJEVIC, D1 2 ; GREBEL, E. K2 ; COLE, A. A3
[1] Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, EH9 3HJ Edinburgh, United Kingdom
[2] Astronomisches Rechen-Institut, Zentrum fur Astronomie der Universitat Heidelberg, Monchhofstrasse 12-14, 69120 Heidelberg, Germany
[3] School of Mathematics & Physics, University of Tasmania, Private Bag 37 Hobart, 7001 Tasmania, Australia
Source

Astronomy and astrophysics (Berlin. Print). 2012, Vol 541 ; A131.1-A131.16 ; 2 ; ref : 3/4 p

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
galaxies: dwarf galaxies: evolution galaxies: groups: individual: Centaurus A galaxies: photometry galaxies: stellar content
Keyword (fr)
Activité stellaire Contenu stellaire Diagramme magnitude couleur Durée vie Evolution galaxies Formation stellaire Galaxies irrégulières Galaxies naines Groupe galaxies Groupe local Luminosité Métallicité Photométrie Propriété physique Taux formation
Keyword (en)
Stellar activity Stellar content Color-magnitude diagrams Lifetime Galaxy evolution Star formation Irregular galaxies Dwarf galaxies Galaxy groups Local group Luminosity Metallicity Photometry Physical properties Formation rate
Keyword (es)
Contenido estelar Evolución galaxias Metalicidad Grado formación
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
26196458

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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