Please use this identifier to cite or link to this item:
Full metadata record
DC FieldValueLanguage
dc.contributor.authorDatta, B-
dc.contributor.authorKapoor, R. C-
dc.identifier.citationAstrophysical Journal, Vol. 331, No. 2, Part 1, pp. 784 - 793en
dc.description.abstractResults 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.en
dc.publisherThe American Astronomical Societyen
dc.subjectGravitational Effectsen
dc.subjectNeutron Starsen
dc.subjectSpectral Line Widthen
dc.subjectStellar Radiationen
dc.subjectStellar Rotationen
dc.subjectDoppler Effecten
dc.subjectEmission Spectraen
dc.subjectGamma Ray Burstsen
dc.subjectStellar Massen
dc.titleLimits on rotation-induced characteristics of radiation from stable rapidly rotating neutron starsen
Appears in Collections:IIAP Publications

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.