dc.contributor.author |
Datta, B |
|
dc.contributor.author |
Kapoor, R. C |
|
dc.date.accessioned |
2008-09-17T11:45:41Z |
|
dc.date.available |
2008-09-17T11:45:41Z |
|
dc.date.issued |
1988-08 |
|
dc.identifier.citation |
Astrophysical Journal, Vol. 331, No. 2, Part 1, pp. 784 - 793 |
en |
dc.identifier.issn |
0004-637X |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3703 |
|
dc.description.abstract |
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. |
en |
dc.language.iso |
en |
en |
dc.publisher |
The American Astronomical Society |
en |
dc.relation.uri |
http://ads.ari.uni-heidelberg.de/abs/1988ApJ...331..784D |
en |
dc.subject |
Gravitational Effects |
en |
dc.subject |
Neutron Stars |
en |
dc.subject |
Spectral Line Width |
en |
dc.subject |
Stellar Radiation |
en |
dc.subject |
Stellar Rotation |
en |
dc.subject |
Doppler Effect |
en |
dc.subject |
Emission Spectra |
en |
dc.subject |
Gamma Ray Bursts |
en |
dc.subject |
Stellar Mass |
en |
dc.title |
Limits on rotation-induced characteristics of radiation from stable rapidly rotating neutron stars |
en |
dc.type |
Article |
en |