Discovery of the spectroscopic binary nature of three bright southern Cepheids

Szabados, László and Anderson, R. I. and Derekas, Aliz and Kiss, L. László and Szalai, Tamás and Székely, Péter and Christiansen, J. L. (2013) Discovery of the spectroscopic binary nature of three bright southern Cepheids. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 434 (1). pp. 870-877. ISSN 0035-8711

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Abstract

We present an analysis of spectroscopic radial velocity and photometric data of three bright Galactic Cepheids: LR Trianguli Australis (LR TrA), RZ Velorum (RZ Vel), and BG Velorum (BG Vel). Based on new radial velocity data, these Cepheids have been found to be members of spectroscopic binary systems. The ratio of the peak-to-peak radial velocity amplitude to photometric amplitude indi- cates the presence of a companion for LR TrA and BG Vel. IUE spectra indicate that the companions of RZ Vel and BG Vel cannot be hot stars. The analysis of all available photometric data revealed that the pulsation period of RZ Vel and BG Vel varies monotonically, due to stellar evolution. Moreover, the longest period Cepheid in this sample, RZ Vel, shows period fluctuations superimposed on the monotonic period increase. The light-time effect interpretation of the observed pattern needs long-term photometric monitoring of this Cepheid. The pulsation period of LR TrA has remained con- stant since the discovery of its brightness variation. Using statistical data, it is also shown that a large number of spectroscopic binaries still remain to be discovered among bright classical Cepheids.

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