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http://hdl.handle.net/2289/2747
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DC Field | Value | Language |
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dc.contributor.author | Srinivasan, G. | - |
dc.date.accessioned | 2007-06-11T11:16:14Z | - |
dc.date.available | 2007-06-11T11:16:14Z | - |
dc.date.issued | 1990 | - |
dc.identifier.citation | Advances in Space Research, 1990, Vol.10, p167-178 | en |
dc.identifier.issn | 0273-1177 | - |
dc.identifier.uri | http://hdl.handle.net/2289/2747 | - |
dc.description | Restricted Access. | en |
dc.description.abstract | A discussion is presented focusing on the origin of millisecond pulsars as part of a continuing effort in finding out whether or not they are gamma ray emitters. It is proposed that there may be as many as 10,000 millisecond pulsars throughout the Galaxy, as suggested by fairly conservative scaling. If so, then they may make a significant contribution to the gamma ray background. The discussion concludes with a speculation regarding the recently discovered 1.6 millisecond eclipsing binary pulsar. | en |
dc.format.extent | 797040 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Elsevier B.V. | en |
dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?1990AdSpR..10..167S | en |
dc.relation.uri | http://dx.doi.org/10.1016/0273-1177(90)90137-O | en |
dc.rights | 1990 Elsevier B.V. | en |
dc.subject | Gamma ray astronomy | en |
dc.subject | Pair production | en |
dc.subject | Pulsar magnetospheres | en |
dc.subject | Pulsars | en |
dc.subject | X-ray binaries | en |
dc.subject | Astronomical models | en |
dc.subject | Stellar evolution | en |
dc.subject | Stellar magnetic fields | en |
dc.subject | Stellar rotation | en |
dc.title | Millisecond pulsars - A new population of gamma ray sources? | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1990 Adv Space Res V10 p167.pdf Restricted Access | Restricted Access | 778.36 kB | Adobe PDF | View/Open Request a copy |
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