Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-20T01:29:51.304Z Has data issue: false hasContentIssue false

Cepheid Variables in the LMC and SMC

Published online by Cambridge University Press:  25 May 2016

D.L. Welch
Affiliation:
Dept. of Physics & Astronomy, McMaster University, Hamilton, Ontario, L8S 4M1 Canada

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.

In this paper, we will review major new results regarding classical Cepheids, in the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC). Specifically, we discuss recent work regarding multimode Cepheids and describe new observations of a W Vir star (HV 5756) and a Cepheid which are each in eclipsing binary systems. An additional interesting pulsating supergiant in an eclipsing system is also identified. Ephemerides for eclipses for the three systems are provided.

Type
Part 8. Cepheids and Distances
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Alcock, C. et al. 1999a, AJ, in press Google Scholar
Alcock, C. et al. 1999b, ApJ, in press Google Scholar
Beaulieu, J.-P. et al. 1997, A&A, 321, L5 Google Scholar
Bersier, D. 1998, A.S.P. Conf. Series, 135, 24 Google Scholar
Cook, K.H. et al. 1997, Proc. 12th I.A.P., 17 Google Scholar
Rorabeck, A. 1997, , Google Scholar
Welch, D.L., 1998, A.S.P. Conf. Series, 135, 355 Google Scholar
Welch, D.L., et al. 1998, I.A.U. Circular 6802 Google Scholar
Welch, D.L., et al. 1996, I.A.U. Circular 6434 Google Scholar