Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-12T18:38:09.513Z Has data issue: false hasContentIssue false
  • English
  • Français

Pulsating Stars and Other Variables in h and χ Persei

Published online by Cambridge University Press:  12 April 2016

J. Krzesiński  and
A. Pigulski
J. Krzesiński
Affiliation:
Mt. Suhora Observatory, Cracow Pedagogical University, ul. Podchorqżych 2, 30-084 Kraków, PolandDepartment of Astronomy, University of Cape Town, Rondebosch 7700, Cape Town, South Africa
A. Pigulski
Affiliation:
Wroclaw University Observatory, ul. Kopernika 1, 51-622 Wroclaw, Poland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present the current status of the ongoing search for B-type pulsators in the double cluster h and χ Persei.

Type
Part 6. Variables Close to the Main Sequence
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 496
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Krzesiński, J. & Pigulski, A. 1997, A&A, 325, 987 Google Scholar
Krzesiński, J., Pigulski, A., & Kołaczkowski, Z. 1999, A&A, 345, 505 Google Scholar
Oosterhoff, P.T. 1937, Leiden Ann., 17, 1 Google Scholar