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Photometric observations of RCB stars In the LMC

Published online by Cambridge University Press:  12 April 2016

W.A. Lawson  and
P.L. Cottrell
W.A. Lawson
Affiliation:
Mount John University Observatory, Department of Physics, University of Canterbury, Christchurch, New Zealand
P.L. Cottrell
Affiliation:
Mount John University Observatory, Department of Physics, University of Canterbury, Christchurch, New Zealand

Extract

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We present UBV photometric observations of two R Coronae Borealis (RCB) stars, W Mensae and HV12842, which are members of the Large Magallenic Cloud (LMC). These data have been obtained over the last two years using single-channel photometers on both the 0.6m and lm telescopes at Mount John. They form part of an ongoing long-term program to investigate photometric and spectroscopic variations in the hydrogen-deficient carbon (HdC) stars both in the LMC and in our Galaxy.

Type
1. Properties and Kinematics of the Peculiar Red Giant Stars
Information
International Astronomical Union Colloquium , Volume 106: Evolution of Peculiar Red Giant Stars , 1989 , pp. 57
Copyright
Copyright © Cambridge University Press 1989