Precession of the rotation axis of the pulsar PSR 1913 + 16

Details Precession of the rotation axis of the pulsar PSR 1913 + 16 Precession of the rotation axis of the pulsar PSR 1913 + 16

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..711i&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, Aug. 1991, p. 711-718. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Binary Stars, Companion Stars, Neutron Stars, Pulsars, Stellar Magnetospheres, Axes Of Rotation, Precession, Radio Emission, Stellar Rotation

Scientific paper

Data observed at a frequency of 1408 MHz are used to determine the precession parameters for PSR 1913 + 16. The precession angle is 25 deg, which is consistent with the notion that the binary system of neutron stars incorporating the pulsar was formed as a result of the explosion of the progenitor of the companion's star. The precession makes it possible to observe the entire region of radio wave generation in the magnetosphere of PSR 1913 + 16.

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