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How to disentangle the group of dwarf elliptical galaxies in the Virgo cluster
Author(s) -
Gotthart T.,
Jäger M.,
Hensler G.,
Zeilinger W.W.,
Boselli A.
Publication year - 2009
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.200911288
Subject(s) - virgo cluster , physics , astrophysics , sky , dwarf galaxy , galaxy , cluster (spacecraft) , elliptical galaxy , galaxy cluster , galaxy group , brightest cluster galaxy , astronomy , computer science , programming language
A sample of early‐type dwarf galaxies of the Virgo cluster extracted from the Sloan Digital Sky Survey is analyzed to search for two different populations: galaxies which were formed in the cluster and galaxies which were accreted at a later stage and which were stripped during this process. Photometric and spectroscopic data has been used for the analysis. Due to the low signal‐to‐noise ratios of the data, the results are however inconclusive (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

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