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http://hdl.handle.net/2248/4187| Title: | Disk Luminosity for Accreting, Weak Magnetic Field Neutron Stars in the ``Slow'' Rotation Approximation |
| Authors: | Datta, B |
| Issue Date: | 1999 |
| Publisher: | Koninklijke Nederlandse Akademie van Wetenschappen |
| Citation: | Arzoumanian, Z., Van der Hooft, and van den Heuvel, E. P. J., eds., Pulsar Timing, General Relativity and the Internal Structure of Neutron Stars., Published by Koninklijke Nederlandse Akademie van Wetenschappen, Amsterdam, The Netherlands 1999, pp. 287. |
| Abstract: | For accretion onto neutron stars possessing weak surface magnetic fields and substantial rotation rates (corresponding to the secular instability limit), we calculate the disk and surface layer luminosities general relativistically using the Hartle & Thorne formalism, and illustrate these quantities for a set of representative neutron star equations of state. |
| URI: | http://hdl.handle.net/2248/4187 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Disk Luminosity for Accreting | 347.86 kB | Adobe PDF |  View/Open |
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