Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/965
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Deshpande, A.A. | - |
dc.contributor.author | Ramachandran, R. | - |
dc.contributor.author | Srinivasan, G. | - |
dc.date.accessioned | 2005-12-29T06:16:32Z | - |
dc.date.available | 2005-12-29T06:16:32Z | - |
dc.date.issued | 1995 | - |
dc.identifier.citation | Journal of Astrophysics and Astronomy, 1995, Vol. 16, p53-67. | en |
dc.identifier.issn | 0250-6335 | - |
dc.identifier.uri | http://hdl.handle.net/2289/965 | - |
dc.description.abstract | A detailed statistical analysis of pulsar current is presented. The conclusions reached are the following: (1) The birthrate of pulsars is about one in 75 ± 15 years. (2) There is evidence for injection of pulsars into the population of solitary pulsars. Such an injection is particularly pronounced in the magnetic field range 12 < log B < 12.6. (3) This is interpreted as due to recycled pulsars being released into the population. (4) We tentatively conclude that as much as 10-15% of all pulsars may have been born and processed in binary systems. | en |
dc.format.extent | 1235847 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Indian Academy of Sciences, Bangalore, India. | en |
dc.rights | Indian Academy of Sciences, Bangalore, India. | en |
dc.subject | Pulsars; | en |
dc.subject | Stars: evolution; | en |
dc.subject | Stars: magnetic; | en |
dc.subject | Stars: stellar statistics | en |
dc.title | Are many pulsars processed in binary systems? | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1995_JAA_V16_p53-67.pdf | 15p. | 1.21 MB | Adobe PDF | View/Open |
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.