Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/3978
Title: | A model for the millisecond pulsar PSR 1937 + 214 |
Authors: | Kochhar, R. K Sivaram, C |
Keywords: | Astrophysics Binary Stars Pulsars Stellar Models Angular Momentum Momentum Transfer Neutron Stars Stellar Mass Accretion |
Issue Date: | Jan-1984 |
Publisher: | Springer |
Citation: | Astrophysics and Space Science, Vol. 98, No. 1, pp. 201- 202 |
Abstract: | The authors suggest a model for the millisecond pulsar PSR 1937+214, according to which the immediate progenitor of the pulsar was a binary consisting of two neutron stars of unequal mass. The heavier neutron star was spun up by the transfer of angular momentum from the orbit, and the lighter neutron star was tidally disrupted, leaving behind a millisecond pulsar. |
URI: | http://hdl.handle.net/2248/3978 |
ISSN: | 0004-640X |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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On the slow-down of the millisecond pulsar PSR 1937 + 214 | 221.37 kB | Adobe PDF | View/Open |
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