Rasio, F. A. and Shapiro, S. L. and Teukolsky, S. A. (1992) Formation of a 'planet' by rapid evaporation of a pulsar's companion. Astronomy and Astrophysics, 256 (2). L35-L37. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20180606-165035387
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Abstract
A planet-size object in circular orbit around a pulsar could be formed as the result of rapid evaporation of a more massive binary companion by the pulsar's radiation.
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| Additional Information: | © European Southern Observatory 1992. Received December 24, 1991; accepted January 10, 1992. We thank L. Bildsten for a useful conversation, A. Thoul for a critical reading of the manuscript, and I. Wasserman for comments. This work has been supported in part by NSF grants AST90-15451 and PHY90-07834, and NASA grant NAGW-2364 to Cornell University. | ||||||||
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| Subject Keywords: | pulsars - stars: planetary systems | ||||||||
| Issue or Number: | 2 | ||||||||
| Record Number: | CaltechAUTHORS:20180606-165035387 | ||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20180606-165035387 | ||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||
| ID Code: | 86874 | ||||||||
| Collection: | CaltechAUTHORS | ||||||||
| Deposited By: | George Porter | ||||||||
| Deposited On: | 07 Jun 2018 21:41 | ||||||||
| Last Modified: | 09 Mar 2020 13:19 |
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