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| Query : 2004MNRAS.354L..49S |
2004MNRAS.354L..49S - Mon. Not. R. Astron. Soc., 354, L49-L53 (2004/November-2)
Recycled pulsars with black hole companions: the high-mass analogues of PSR B2303+46.
SIPIOR M.S., PORTEGIES ZWART S. and NELEMANS G.
Abstract (from CDS):
An estimate of the formation rate through this channel is first performed via a simple analytical approach, and then refined using the results of the SeBa binary evolution package. The central role of kicks in determining the survival rate of these binaries is clearly demonstrated. The final result is expressed in terms of the number of field pulsars one can expect for every single neutron star-black hole (ns, bh) binary. We also calculate this figure for black hole-neutron star (bh, ns) systems formed through the usual channel. Assuming kicks drawn from the distribution of Cordes & Chernoff, we find an expectation value of one (ns, bh) binary per 4x104 pulsars, and one (bh, ns) system for every 1500 pulsars. This helps to explain why neither system has been seen to date, though it suggests that detection of a (bh, ns) binary is imminent.
Abstract Copyright: 2004 RAS
Journal keyword(s): binaries: close - pulsars: general
Simbad objects: 1
| Number of rows : 1 |
| 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 J2305+4707 | Psr | 23 05 55.842 | +47 07 45.32 | ~ | 227 | 1 |
| Query : 2004MNRAS.354L..49S |
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| PSR B2303+46 | PSR J2305+4707 | SBC9 1421 | WEB 20255 |
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References (227 between 1850 and 2026) (Total 227)
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