Radhakrishnan, V. ; Shukre, C. S. (1986) The pulsar velocities and their binary origins (invited review) Astrophysics and Space Science, 118 (1-2). pp. 329-336. ISSN 0004-640X
Full text not available from this repository.
Official URL: http://www.springerlink.com/content/l2742326738677...
Related URL: http://dx.doi.org/10.1007/BF00651146
Abstract
The observed proper-motions are shown to indicate that most pulsars come from binary systems. Due to a remarkable relationship between the speed of a pulsar and that of its progenitor in orbit, it is concluded that these binaries went through a common-envelope phase. This provides independent support to similar conclusions drawn from stellar evolution considerations.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Springer. |
| ID Code: | 40770 |
| Deposited On: | 25 May 2011 05:43 |
| Last Modified: | 25 May 2011 05:43 |
Repository Staff Only: item control page
