Journal
ASTROPHYSICAL JOURNAL LETTERS
Volume 740, Issue 2, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/2041-8205/740/2/L47
Keywords
binaries: close; open clusters and associations: individual (NGC 6791); stars: horizontal-branch; stars: oscillations
Categories
Funding
- NASA's Science Mission Directorate
- National Aeronautics and Space Administration [NNX11AC74G, 09-KEPLER09-0056]
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We report on Kepler photometry of the hot subdwarf B (sdB) star B4 in the open cluster NGC 6791. We confirm that B4 is a reflection effect binary with an sdB component and a low-mass main-sequence companion with a circular 0.3985 day orbit. The sdB star is a g-mode pulsator (a V1093 Her star) with periods ranging from 2384 s to 7643 s. Several of the pulsation modes show symmetric splitting by 0.62 mu Hz. Attributing this to rotational splitting, we conclude that the sdB component has a rotation period of approximately 9.63 days, indicating that tidal synchronization has not been achieved in this system. Comparison with theoretical synchronization time provides a discriminant between various theoretical models.
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