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Abstract
The birth kicks of black holes, arising from asymmetric mass ejection or neutrino emission during core-collapse supernovae, are of great interest for both observationally constraining supernova models and population-synthesis studies of binary evolution. Recently, several efforts were undertaken to estimate black hole birth kicks from observations of black hole low-mass X-ray binaries. We follow up on this work, specifically focusing on the highest estimated black hole kick velocities. We find that existing observations do not require black hole birth kicks in excess of approximately 80 km s−1, although higher kicks are not ruled out.
Original language | English |
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Pages (from-to) | 578-581 |
Journal | Royal Astronomical Society. Monthly Notices |
Volume | 456 |
Issue number | 1 |
DOIs | |
Publication status | Published - 11 Feb 2016 |
Keywords
- binaries: close
- stars: black holes
- Galaxy: kinematics and dynamics
- X-rays: binaries
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Dive into the research topics of 'Estimates of black hole natal kick velocities from observations of low-mass X-ray binaries'. Together they form a unique fingerprint.Projects
- 1 Finished
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Birmingham Astrophysics : Consolidated Grant 2013-2016
Vecchio, A., Ponman, T., Freise, A., Smith, G., Speake, C., Mandel, I., Cruise, M., Raychaudhury, S. & Stevens, I.
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/04/13 → 30/09/16
Project: Research Councils