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Variable Stars in the Holmberg II Dwarf Galaxy* **

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© 1998. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
, , Citation John G. Hoessel et al 1998 AJ 115 573 DOI 10.1086/300214

1538-3881/115/2/573

Abstract

     The dwarf irregular galaxy Holmberg II (DDO 50) has been observed on 34 separate nights for the purpose of finding and photometering variable stars. Extensive analysis of the CCD frames obtained over 14 years has yielded a set of 28 candidate pulsating variable stars that are likely to be Cepheids. Further selection based on available colors defines a set of seven very likely Cepheids. Comparison of these data with the period-luminosity relation of Madore & Freedman for Magellanic Cloud Cepheids produces a distance modulus of m - M = 27.42, which corresponds to 3.05 Mpc.

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Footnotes

  • Observations obtained at Kitt Peak National Observatory, National Optical Astronomy Observatories, operated by the Association of Universities for Research in Astronomy (AURA), Inc., under cooperative agreement with the National Science Foundation.

  • ** 

    Observations obtained at the Palomar Observatory, California Institute of Technology.

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10.1086/300214