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Cepheids and LPVs in and around Magellanic Cloud Clusters

Published online by Cambridge University Press:  12 April 2016

K.M. Sebo  and
P.R. Wood
K.M. Sebo
Affiliation:
Mount Stromlo & Siding Spring Observatories, Private Bag, Weston Creek PO, Canberra ACT 2611, Australia
P.R. Wood
Affiliation:
Mount Stromlo & Siding Spring Observatories, Private Bag, Weston Creek PO, Canberra ACT 2611, Australia

Abstract

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V and I band CCD photometry of the young clusters NGC 330 (SMC), NGC 1850, NGC 2058 and NGC 2065 (LMC) has been used to find variable stars in and around the clusters. The variables detected are mostly Cepheids and long-period variables (LPVs). Here we outline some results of these studies.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 383 - 384
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

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