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http://hdl.handle.net/2248/3703| Title: | Limits on rotation-induced characteristics of radiation from stable rapidly rotating neutron stars |
| Authors: | Datta, B Kapoor, R. C |
| Keywords: | Gravitational Effects Neutron Stars Spectral Line Width Stellar Radiation Stellar Rotation Doppler Effect Emission Spectra Gamma Ray Bursts Stellar Mass |
| Issue Date: | Aug-1988 |
| Publisher: | The American Astronomical Society |
| Citation: | Astrophysical Journal, Vol. 331, No. 2, Part 1, pp. 784 - 793 |
| 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. |
| URI: | http://hdl.handle.net/2248/3703 |
| ISSN: | 0004-637X |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Limits on rotation-induced characteristics of radiation from stable rapidly rotating neutron stars | 1.15 MB | Adobe PDF | View/Open |
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