Published September 1994
| Published
Journal Article
Open
Binary and Millisecond Pulsars
- Creators
-
Phinney, E. S.
-
Kulkarni, S. R.
Abstract
Most of the ~600 known pulsars are single and located in the disk of our Galaxy. There is circumstantial evidence that the pulsars in this majority are created in supernova (SN) explosions, by the collapse of the cores of massive stars (initial mass M_i ≳ M_(cr) ≃ 8 M_⊙). One is created roughly every 100 y in the Galaxy.
Additional Information
© 1994 by Annual Reviews Inc. ESP was partly supported by NASA Astrophysics Theory grant NAGW-2394 and the Alfred P. Sloan Foundation. SRK's work was supported by NASA, NSF, and the Packard Foundation.Attached Files
Published - PHIaraa94.pdf
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PHIaraa94.pdf
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Additional details
- Eprint ID
- 29424
- Resolver ID
- CaltechAUTHORS:20120223-080709481
- NAGW-2394
- NASA
- Alfred P. Sloan Foundation
- NSF
- David and Lucile Packard Foundation
- Created
-
2012-02-29Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- TAPIR, Division of Geological and Planetary Sciences