The Runaway Binary LP 400-22 is Leaving the Galaxy

Monthly Notices of the Royal Astronomical Society(2013)

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摘要
We present optical spectroscopy, astrometry, radio and X-ray observations of the runaway binary LP 400−22. We refine the orbital parameters of the system based on our new radial velocity observations. Our parallax data indicate that LP 400−22 is significantly more distant (3σ lower limit of 840 pc) than initially predicted. LP 400−22 has a tangential velocity in excess of 830 km s−1; it is unbound...
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关键词
binaries: close,stars: individual: LP 400−22,stars: individual: WD 2234+222,white dwarfs,Galaxy: kinematics and dynamics,Galaxy: stellar content
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