A Common Proper Motion Stellar Companion to HAT-P-7
We report that HAT-P-7 has a common proper motion stellar companion. The companion is located at $ \sim$ 3 $ .\!\!\!''$ 9 to the east and estimated to be an M5.5V dwarf based on its colors. We also confirm the presence of a third companion, which was first reported by Winn et al. (2009, Ap...
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Veröffentlicht in: | Publications of the Astronomical Society of Japan 2012-12, Vol.64 (6) |
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Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
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Zusammenfassung: | We report that HAT-P-7 has a common proper motion stellar companion. The companion is located at
$ \sim$
3
$ .\!\!\!''$
9 to the east and estimated to be an M5.5V dwarf based on its colors. We also confirm the presence of a third companion, which was first reported by Winn et al. (2009, ApJ, 703, L99), based on long-term radial velocity measurements. We revisit the migration mechanism of HAT-P-7b given to the presence of those companions, and propose the sequential Kozai migration as a likely scenario in this system. This scenario may explain the reason for an outlier in the discussion of the spin-orbit alignment timescale for HAT-P-7b by Albrecht et al. (2012, ApJ, 757, 18). |
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ISSN: | 0004-6264 2053-051X |
DOI: | 10.1093/pasj/64.6.L7 |