2004MNRAS.354L..49S


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):

We investigate the possibility that mass transfer early in the evolution of a massive binary can effect a reversal of the end states of the two components, resulting in a neutron star that forms before a black hole. In this sense, such systems would comprise the high-mass analogues of white dwarf-neutron star systems such as PSR B2303+46. One consequence of this reversal is that a second episode of mass transfer from the black hole progenitor star can recycle the nascent neutron star, extending the life of the pulsar.

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

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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

Basic data :
PSR J2305+4707 -- Pulsar
Other object types:
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Psr (PSR), SB* (SBC9), * (WEB)
ICRS coord. (ep=J2000) :
23 05 55.842 +47 07 45.32 [ ] D 1993ApJ...405L..29T
FK4 coord. (ep=B1950 eq=1950) :
23 03 39.161 +46 51 32.22 [ ]
Gal coord. (ep=J2000) :
104.930748 -12.021382 [ ]
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Identifiers (4) :
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PSR B2303+46 PSR J2305+4707 SBC9 1421 WEB 20255

References (227 between 1850 and 2026) (Total 227)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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