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arXiv · 1103.3070

Spectroscopy of BL Cam - Observations

M. Alvarez·R. Michel·L. Fox-Machado·J. P. Sareyan·S. Fauvaud·G. Tovmassian
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Abstract

The star BL Camelopardalis (GD 428, GSC 04067-00471, V=12.92, B=13.1), is a SX Phoenicis pulsating variable showing a high amplitude variability (300-350 mmag), with a very clear period of 56.3 min, that has being recently studied by Fauvaud et al. (2010). They show that the observed variability is due to a clear and single pulsation, as expected for these type of pulsators. It was discovered as a variable star on 1976 by Berg and Duthie (1977).

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M. Alvarez, R. Michel, L. Fox-Machado, J. P. Sareyan, S. Fauvaud, G. Tovmassian. 2011-03-16. Spectroscopy of BL Cam - Observations. https://arxiv.org/abs/1103.3070

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