The Pulsation Period of the Hot Hydrogen-Deficient Star MV Sgr

Details The Pulsation Period of the Hot Hydrogen-Deficient Star MV Sgr The Pulsation Period of the Hot Hydrogen-Deficient Star MV Sgr

2012-02-27

arxiv.org/abs/1202.6040v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Scientific paper

MV Sgr is a hot, hydrogen-deficient star which has undergone R CrB fadings.
We have used self-correlation analysis and Fourier analysis of CCD V photometry
in the AAVSO International Database to identify a period of 8.0 days in this
star; the amplitude is about 0.03 mag. The variability is most likely due to
pulsation.

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