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Substructure in dwarf spheroidals: a star cluster connection?

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Substructure in dwarf spheroidals: a star cluster connection? / Wilkinson, M. I.; Kleyna, Jan; Evans, N. W. et al.
In: Proceedings of the International Astronomical Union, Vol. 1, No. C198, 2005, p. 240-243.

Research output: Contribution to Journal/Magazine › Journal article

Harvard

Wilkinson, MI, Kleyna, J, Evans, NW, Gilmore, G, Grebel, EK, Koch, A, Read, J & Young, R 2005, 'Substructure in dwarf spheroidals: a star cluster connection?', Proceedings of the International Astronomical Union, vol. 1, no. C198, pp. 240-243. https://doi.org/10.1017/S1743921305003819

APA

Wilkinson, M. I., Kleyna, J., Evans, N. W., Gilmore, G., Grebel, E. K., Koch, A., Read, J., & Young, R. (2005). Substructure in dwarf spheroidals: a star cluster connection? Proceedings of the International Astronomical Union, 1(C198), 240-243. https://doi.org/10.1017/S1743921305003819

Vancouver

Wilkinson MI, Kleyna J, Evans NW, Gilmore G, Grebel EK, Koch A et al. Substructure in dwarf spheroidals: a star cluster connection? Proceedings of the International Astronomical Union. 2005;1(C198):240-243. doi: 10.1017/S1743921305003819

Author

Wilkinson, M. I. ; Kleyna, Jan ; Evans, N. W. et al. / Substructure in dwarf spheroidals : a star cluster connection?. In: Proceedings of the International Astronomical Union. 2005 ; Vol. 1, No. C198. pp. 240-243.

Bibtex

@article{7be95c493b0c4574b9164cb4fb8b5740,
title = "Substructure in dwarf spheroidals: a star cluster connection?",
abstract = "The observational evidence for kinematic substructure in Local Group dSphs is reviewed. The properties of these substructures are consistent with their being disrupted star clusters. The persistence of cold substructure argues strongly against the presence of dark matter cusps in the haloes of dSphs. A formation scenario for dSphs is described involving the merger of star clusters in the potential well of a low-mass dark matter halo.",
author = "Wilkinson, {M. I.} and Jan Kleyna and Evans, {N. W.} and G. Gilmore and Grebel, {E. K.} and Andreas Koch and Justin Read and R. Young",
year = "2005",
doi = "10.1017/S1743921305003819",
language = "English",
volume = "1",
pages = "240--243",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "C198",

}

RIS

TY - JOUR

T1 - Substructure in dwarf spheroidals

T2 - a star cluster connection?

AU - Wilkinson, M. I.

AU - Kleyna, Jan

AU - Evans, N. W.

AU - Gilmore, G.

AU - Grebel, E. K.

AU - Koch, Andreas

AU - Read, Justin

AU - Young, R.

PY - 2005

Y1 - 2005

N2 - The observational evidence for kinematic substructure in Local Group dSphs is reviewed. The properties of these substructures are consistent with their being disrupted star clusters. The persistence of cold substructure argues strongly against the presence of dark matter cusps in the haloes of dSphs. A formation scenario for dSphs is described involving the merger of star clusters in the potential well of a low-mass dark matter halo.

AB - The observational evidence for kinematic substructure in Local Group dSphs is reviewed. The properties of these substructures are consistent with their being disrupted star clusters. The persistence of cold substructure argues strongly against the presence of dark matter cusps in the haloes of dSphs. A formation scenario for dSphs is described involving the merger of star clusters in the potential well of a low-mass dark matter halo.

U2 - 10.1017/S1743921305003819

DO - 10.1017/S1743921305003819

M3 - Journal article

VL - 1

SP - 240

EP - 243

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - C198

ER -