Published March 1992
| Published
Journal Article
Open
Formation of a 'planet' by rapid evaporation of a pulsar's companion
- Creators
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Rasio, F. A.
- Shapiro, S. L.
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Teukolsky, S. A.
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.
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.Attached Files
Published - 1992A+A___256L__35R.pdf
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1992A+A___256L__35R.pdf
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Additional details
- Eprint ID
- 86874
- Resolver ID
- CaltechAUTHORS:20180606-165035387
- AST90-15451
- NSF
- PHY90-07834
- NSF
- NAGW-2364
- NASA
- Created
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2018-06-07Created from EPrint's datestamp field
- Updated
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2020-03-09Created from EPrint's last_modified field