Limits on rotation-induced characteristics of radiation from stable rapidly rotating neutron stars

Details Limits on rotation-induced characteristics of radiation from stable rapidly rotating neutron stars Limits on rotation-induced characteristics of radiation from stable rapidly rotating neutron stars

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...331..784d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 331, Aug. 15, 1988, p. 784-793.

Astronomy and Astrophysics

Astrophysics

3

Gravitational Effects, Neutron Stars, Spectral Line Width, Stellar Radiation, Stellar Rotation, Doppler Effect, Emission Spectra, Gamma Ray Bursts, Stellar Mass

Scientific paper

Results are presented of a study of frequency shifts in radiation from the surface of rapidly rotating neutron stars and rotation-induced spectral line broadening as a function of their mass. It is found that, despite large rotation rates, the gravitational effects dominate over the Doppler contribution to the frequency shifts over the allowed mass range of a stable rotating neutron star. Astrophysical implications of effect of large rotation on spectral line characteristics are also discussed.

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