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http://hdl.handle.net/2289/744
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DC Field | Value | Language |
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dc.contributor.author | Bhattacharya, D. | - |
dc.contributor.author | Srinivasan, G. | - |
dc.date.accessioned | 2005-12-16T09:25:59Z | - |
dc.date.available | 2005-12-16T09:25:59Z | - |
dc.date.issued | 1991-02-11 | - |
dc.identifier.citation | Journal of Astrophysics and Astronomy, 1991, Vol. 12, p17-25. | en |
dc.identifier.issn | 0250-6335 | - |
dc.identifier.uri | http://hdl.handle.net/2289/744 | - |
dc.description.abstract | The contribution of millisecond pulsars to the diffuse gamma-ray background of the Galaxy is estimated, and it is shown that a significant fraction of the Galactic background may originate from them. A small number of the unidentified COS-B point sources may, in fact, be millisecond pulsars. It is argued that several hundred millisecond pulsars may be detectable as point sources by the GRO satellite. | en |
dc.format.extent | 789791 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 | Millisecond-gamma-ray emission | en |
dc.subject | Diffuse gamma- ray background | en |
dc.title | Gamma rays from millisecond pulsars. | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1991_JAA_V12_p17-25.pdf | 9p. | 771.28 kB | Adobe PDF | View/Open |
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