Dwarf spheroidals in the M81 galaxy group

Physics

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Dwarf spheroidals in the M81 galaxy group. / Lianou, S.; Grebel, E. K.; Koch, Andreas.
In: ASP Conference Series, Vol. 424, 2010, p. 242-243.

Research output: Contribution to Journal/Magazine › Journal article

Harvard

Lianou, S, Grebel, EK & Koch, A 2010, 'Dwarf spheroidals in the M81 galaxy group', ASP Conference Series, vol. 424, pp. 242-243. <http://www.aspbooks.org/a/volumes/article_details/?paper_id=31388>

APA

Lianou, S., Grebel, E. K., & Koch, A. (2010). Dwarf spheroidals in the M81 galaxy group. ASP Conference Series, 424, 242-243. http://www.aspbooks.org/a/volumes/article_details/?paper_id=31388

Vancouver

Lianou S, Grebel EK, Koch A. Dwarf spheroidals in the M81 galaxy group. ASP Conference Series. 2010;424:242-243.

Author

Lianou, S. ; Grebel, E. K. ; Koch, Andreas. / Dwarf spheroidals in the M81 galaxy group. In: ASP Conference Series. 2010 ; Vol. 424. pp. 242-243.

Bibtex

@article{59e707faf32147c0a481b88485711bda,

title = "Dwarf spheroidals in the M81 galaxy group",

abstract = "The M81 group consists of a few large galaxies and about 40 dwarf galaxies. It is a highly interacting group which makes it an important nearby laboratory to study the role of the environment and interactions in the dwarf galaxy formation and evolution. We use the resolved stellar populations in a sample of early-type dwarf galaxies in this group to derive the photometric metallicity distribution functions and study the potential presence of population gradients in this dwarf galaxy sample.",

author = "S. Lianou and Grebel, {E. K.} and Andreas Koch",

year = "2010",

language = "English",

volume = "424",

pages = "242--243",

journal = "ASP Conference Series",

issn = "1050-3390",

}

RIS

TY - JOUR

T1 - Dwarf spheroidals in the M81 galaxy group

AU - Lianou, S.

AU - Grebel, E. K.

AU - Koch, Andreas

PY - 2010

Y1 - 2010

N2 - The M81 group consists of a few large galaxies and about 40 dwarf galaxies. It is a highly interacting group which makes it an important nearby laboratory to study the role of the environment and interactions in the dwarf galaxy formation and evolution. We use the resolved stellar populations in a sample of early-type dwarf galaxies in this group to derive the photometric metallicity distribution functions and study the potential presence of population gradients in this dwarf galaxy sample.

AB - The M81 group consists of a few large galaxies and about 40 dwarf galaxies. It is a highly interacting group which makes it an important nearby laboratory to study the role of the environment and interactions in the dwarf galaxy formation and evolution. We use the resolved stellar populations in a sample of early-type dwarf galaxies in this group to derive the photometric metallicity distribution functions and study the potential presence of population gradients in this dwarf galaxy sample.

M3 - Journal article

VL - 424

SP - 242

EP - 243

JO - ASP Conference Series

JF - ASP Conference Series

SN - 1050-3390

ER -

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