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The Cepheids Variable Stars Population in the Local Group Dwarf Irregular Galaxy Pegasus
Published online by Cambridge University Press: 01 December 2006
Abstract
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We present the result of a search for Cepheids in the Local Group dwarf irregular galaxy (DIG) Pegasus. We identified 20 Cepheid stars with periods 0d.6 < P < 15d.3. We have compared them with previously published Cepheids and we have carried out an accurate completeness analysis in order to obtain the fraction of them which are lost. Using their period-luminosity relation we obtain a distance for Pegasus of 950±30 Kpc.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 365 - 366
- Copyright
- Copyright © International Astronomical Union 2007
References
Hoessel, J. G., Abbott, M. J., Saha, A., Mossman, A. E. & Danielson, G. E. 1990, AJ 100, 1151CrossRefGoogle Scholar
McConnachie, A. W., Irwin, M. J., Ferguson, A. M. N., Ibata, R. A., Lewis, G. F. & Tanvir, N. 2005, MNRAS 356, 979CrossRefGoogle Scholar
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