PSR J0952−0607: The Fastest and Heaviest Known Galactic Neutron Star
Kavli Institute for Particle Astrophysics and Cosmology · Stanford University · +1 more institution
Abstract
Abstract We describe Keck-telescope spectrophotometry and imaging of the companion of the “black widow” pulsar PSR J0952−0607, the fastest known spinning neutron star (NS) in the disk of the Milky Way. The companion is very faint at minimum brightness, presenting observational challenges, but we have measured multicolor light curves and obtained radial velocities over the illuminated “day” half of the orbit. The model fits indicate system inclination i = 59.°8 ± 1.°9 and a pulsar mass M NS = 2.35 ± 0.17 M ⊙ , the largest well-measured mass found to date. Modeling uncertainties are small, since the heating is not extreme; the companion lies well within its Roche lobe and a simple direct-heating model provides…
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- 72.58
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- References
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Authors
5- RWRoger W. RomaniCorresponding
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University
- DKD. Kandel
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University
- AVA. V. Filippenko
University of California, Berkeley
- TGThomas G. Brink
University of California, Berkeley
- WZWeiKang Zheng
University of California, Berkeley
Topics & keywords
- Physics
- Neutron star
- Astrophysics
- Star (game theory)
- Astronomy
- r-process
- Nucleosynthesis
- Supernova