Direct Statistical Constraints on the Natal Kick Velocity of a Black Hole in an X-Ray Quiet Binary
In recent years, a handful of “dark” binaries have been discovered with a nonluminous compact object. Astrometry and radial velocity measurements of the bright companion allow us to measure the post-supernova orbital elements of such a binary. In this paper, we develop a statistical formalism to use...
المؤلفون الرئيسيون: | , , , , |
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التنسيق: | مقال |
اللغة: | English |
منشور في: |
IOP Publishing
2023-01-01
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سلاسل: | The Astrophysical Journal |
الموضوعات: | |
الوصول للمادة أونلاين: | https://doi.org/10.3847/1538-4357/ad0557 |