On the implications of the submillisecond pulsar in Supernova 1987A

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1126

Full metadata record

DC Field	Value	Language
dc.contributor.author	Bhattacharya, D.	-
dc.contributor.author	Srinivasan, G.	-
dc.date.accessioned	2006-01-09T06:05:07Z	-
dc.date.available	2006-01-09T06:05:07Z	-
dc.date.issued	1989-03-20	-
dc.identifier.citation	Current Science, 1989, Vol. 58, p280-286.	en
dc.identifier.issn	0011-3891	-
dc.identifier.uri	http://hdl.handle.net/2289/1126	-
dc.description.abstract	We discuss the implications of the ultra rapid rotation rate of 1968 Hz of the newly discovered pulsar in supernova 1987A, as well as the sinusoidal modulation of the frequency. It is argued that all the available evidence suggests that the pulsar has a very low magnetic field, about l0^9 G. The significance of this is discussed in detail.	en
dc.format.extent	482303 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 implications of the submillisecond pulsar in Supernova 1987A	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

Files in This Item:

File	Description	Size	Format
1989 CS V58 p280.pdf	7p.	471 kB	Adobe PDF	View/Open