Some characteristics of a rapidly rotating magnetized neutron star

Details Some characteristics of a rapidly rotating magnetized neutron star Some characteristics of a rapidly rotating magnetized neutron star

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983natur.303..409r&link_type=abstract

Nature (ISSN 0028-0836), vol. 303, June 1983, p. 409, 410.

Astronomy and Astrophysics

Astronomy

7

Magnetic Stars, Microwave Spectra, Neutron Stars, Radio Sources (Astronomy), Stellar Models, Stellar Rotation, Gamma Ray Spectra, Spectrum Analysis, Stellar Mass, Stellar Spectrophotometry

Scientific paper

The recently discovered 1.5-ms pulsed radio source PSR 1937+214 could be close to the onset of rotational instabilities if it is envisaged to be a rotating neutron star which gives interesting lower limits for neutron star masses. The authors examine the implications of polar gap models for such a rapidly rotating magnetic neutron star. It appears, on the basis of such models, that a higher fraction of high-frequency microwave radiation compared with the Crab pulsar is an expected result. On the other hand, the outer gap discharge models invoked for longer period pulsars yield a large amount of high-energy radiation which is not observed.

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