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| Query : 2013MNRAS.428.1201B |
2013MNRAS.428.1201B - Mon. Not. R. Astron. Soc., 428, 1201-1206 (2013/January-2)
Periastron advance in neutron star-black hole binaries.
BAGCHI M.
Abstract (from CDS):
As neutron star-black hole binaries are expected to be discovered through future pulsar surveys using upcoming facilities, it is necessary to understand various observable properties of such systems. In this work, we study the advance of the periastron of such binaries under the post-Newtonian formalism over a wide range of parameters. We find that the first- and second-order post-Newtonian effects and the leading order spin-orbit coupling effects are significant for such binaries but higher order effects can be neglected.
Abstract Copyright: © 2012 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society (2012)
Journal keyword(s): gravitation - binaries: close - stars: neutron - pulsars: general
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | PSR J0737-3039 | Psr | 07 37 51.248 | -30 39 40.83 | ~ | 445 | 1 | |||||
| 2 | PSR J1915+1606 | Psr | 19 15 27.99999 | +16 06 27.4034 | 22.5 | ~ | 1032 | 1 |
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