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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3810
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dc.contributor.authorKapoor, R. C-
dc.contributor.authorDatta, B-
dc.date.accessioned2008-09-23T11:04:57Z-
dc.date.available2008-09-23T11:04:57Z-
dc.date.issued1984-08-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 209, No. 4, pp. 895 - 904en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/3810-
dc.description.abstractThe frequency shifts and line broadening of radiation from the surface of rapidly rotating neutron stars are calculated using a rotationally perturbed interior spherical metric and a representative choice of the equation of state for neutron star matter. The effect of rotation on the surface redshift and Doppler broadening are found to be substantial for rotation close to the secular instability limit, relevant for fast pulsars. If gamma-ray line emission originates from the surface of such pulsars, the results presented here can be used to constrain the validity of the equation of state of matter at high densities.en
dc.language.isoenen
dc.publisherThe Royal Astronomical Societyen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1984MNRAS.209..895Ken
dc.subjectNeutron Starsen
dc.subjectRed Shiften
dc.subjectSpectral Line Widthen
dc.subjectStellar Rotationen
dc.subjectStellar Spectraen
dc.subjectEquations Of Stateen
dc.subjectDoppler Effecten
dc.subjectGamma Ray Astronomyen
dc.subjectPulsarsen
dc.subjectStellar Modelsen
dc.titleFrequency shifts and line broadening of radiation from rotating neutron starsen
dc.typeArticleen
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