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M 81 group dSphs: metallicity distribution functions and gradients

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M 81 group dSphs: metallicity distribution functions and gradients. / Lianou, S.; Grebel, E.K.; Koch, Andreas.
In: EAS Publications Series, Vol. 48, 2011, p. 91-92.

Research output: Contribution to Journal/Magazine › Journal article

Harvard

Lianou, S, Grebel, EK & Koch, A 2011, 'M 81 group dSphs: metallicity distribution functions and gradients', EAS Publications Series, vol. 48, pp. 91-92. https://doi.org/10.1051/eas/1148022

APA

Lianou, S., Grebel, E. K., & Koch, A. (2011). M 81 group dSphs: metallicity distribution functions and gradients. EAS Publications Series, 48, 91-92. https://doi.org/10.1051/eas/1148022

Vancouver

Lianou S, Grebel EK, Koch A. M 81 group dSphs: metallicity distribution functions and gradients. EAS Publications Series. 2011;48:91-92. doi: 10.1051/eas/1148022

Author

Lianou, S. ; Grebel, E.K. ; Koch, Andreas. / M 81 group dSphs : metallicity distribution functions and gradients. In: EAS Publications Series. 2011 ; Vol. 48. pp. 91-92.

Bibtex

@article{800d0275da1246ef8e303cd6d15fcf84,
title = "M 81 group dSphs: metallicity distribution functions and gradients",
abstract = "We summarize our results on the photometric metallicities and on the presence of metallicity gradients for nine M 81 group dSphs. The majority of our studied dSphs contains a significant fraction of intermediate–age stellar populations, which we consider as a function of the deprojected distance from the dominant galaxy of the group.",
author = "S. Lianou and E.K. Grebel and Andreas Koch",
year = "2011",
doi = "10.1051/eas/1148022",
language = "English",
volume = "48",
pages = "91--92",
journal = "EAS Publications Series",
issn = "1633-4760",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - M 81 group dSphs

T2 - metallicity distribution functions and gradients

AU - Lianou, S.

AU - Grebel, E.K.

AU - Koch, Andreas

PY - 2011

Y1 - 2011

N2 - We summarize our results on the photometric metallicities and on the presence of metallicity gradients for nine M 81 group dSphs. The majority of our studied dSphs contains a significant fraction of intermediate–age stellar populations, which we consider as a function of the deprojected distance from the dominant galaxy of the group.

AB - We summarize our results on the photometric metallicities and on the presence of metallicity gradients for nine M 81 group dSphs. The majority of our studied dSphs contains a significant fraction of intermediate–age stellar populations, which we consider as a function of the deprojected distance from the dominant galaxy of the group.

U2 - 10.1051/eas/1148022

DO - 10.1051/eas/1148022

M3 - Journal article

VL - 48

SP - 91

EP - 92

JO - EAS Publications Series

JF - EAS Publications Series

SN - 1633-4760

ER -