1998ApJ...509..856K


Query : 1998ApJ...509..856K

1998ApJ...509..856K - Astrophys. J., 509, 856-860 (1998/December-3)

Determination of the geometry of the PSR B1913+16 system by geodetic precession

KRAMER M.

Abstract (from CDS):

New observations of the binary pulsar B1913+16 are presented. Since 1978 the leading component of the pulse profile has weakened dramatically by about 40%. For the first time, a decrease in component separation is observed, consistent with expectations of geodetic precession. Assuming the correctness of general relativity and a circular hollow-cone-like beam, a fully consistent model for the system geometry is developed. The misalignment angle between pulsar spin and orbital momentum is determined, giving direct evidence for an asymmetric kick during the second supernova explosion. It is argued that the orbital inclination angle is 132°.8 (rather than 47°.2). A prediction of this model is that PSR B1913+16 will no longer be observable after the year 2025.

Abstract Copyright: ∼

Journal keyword(s): Stars: Binaries: Close - Stars: Pulsars: Individual: Alphanumeric: B1913+16 - Relativity - Stars: Neutron

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 J1915+1606 Psr 19 15 27.99999 +16 06 27.4034     22.5     ~ 1032 1

Query : 1998ApJ...509..856K

Basic data :
PSR J1915+1606 -- Pulsar
Other object types:
otypes_help
SB* (SBC7,SBC9), Psr (PSR), * (WEB)
ICRS coord. (ep=J2000) :
19 15 27.99999 +16 06 27.4034 [ ] D 2003ASPC..302...93W
FK4 coord. (ep=B1950 eq=1950) :
19 13 12.45366 +16 01 07.9874 [ ]
Gal coord. (ep=J2000) :
049.96765583 +02.12189140 [ ]
Fluxes (1) :
V 22.5 [~] E ~
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notes:


Identifiers (7) :
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PSR B1913+16.0 PSR B1913+16 SBC7 741 WEB 16499
NAME Hulse-Taylor PSR PSR J1915+1606 SBC9 1137

References (1032 between 1850 and 2026) (Total 1032)
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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