Abstract
We present observations of two new single-lined eclipsing binaries, both consisting of an Am star and an M-dwarf, discovered by the Wide Angle Search for Planets transit photometry survey. Using WASP photometry and spectroscopic measurements we find that HD 186753B has an orbital period of P=1.9194 days, a mass of M=0.24plusmn0.02M$_⊙$ and radius of R=0.31$^+0.06$$_-0.06$R$_⊙$; and that TCY7096-222-1B has an orbital period of P=8.9582 days, a mass of between 0.29 and 0.54 M$_⊙$ depending on eccentricity and radius of R=0.263$^+0.02$$_-0.07$R$_⊙$. We find that the Am stars have relatively low rotational velocities that closely match the orbital velocities of the M-dwarfs, suggesting that they have been ldquospun-downrdquo by the M-dwarfs.
Original language | English |
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Pages (from-to) | 391-394 |
Number of pages | 4 |
Journal | Astronomy and Astrophysics |
Volume | 508 |
DOIs | |
Publication status | Published - 1 Dec 2009 |
Keywords
- binaries: eclipsing, stars: early-type, stars: late-type, stars: individual: HD 186753, stars: individual: TCY7096-222-1