Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/1084
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Bhattacharya, D. | - |
dc.contributor.author | Srinivasan, G. | - |
dc.date.accessioned | 2006-01-04T10:52:16Z | - |
dc.date.available | 2006-01-04T10:52:16Z | - |
dc.date.issued | 1986-04-05 | - |
dc.identifier.citation | Current Science, 1986, Vol. 55, p327-330. | en |
dc.identifier.issn | 0011-3891 | - |
dc.identifier.uri | http://hdl.handle.net/2289/1084 | - |
dc.description.abstract | We argue that the extraordinary fact that all three known millisecond pulsars are very close to the galactic plane implies that there must be ~100 potentially observable millisecond pulsars within ~ 4 kpc from the Sun. Our other main conclusion is that the dipole magnetic fields of old neutron stars probably saturate around 5 x l0^8 gauss. | en |
dc.format.extent | 265748 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.title | On the implication of the recently discovered 5 millisecond binary pulsar PSR 1855+09 | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1986 CS V55 p327.pdf | 4p. | 259.52 kB | Adobe PDF | View/Open |
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.