The case for no field decay from improved pulsar population studies

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2423

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DC Field	Value	Language
dc.contributor.author	Hartman, J.W.	-
dc.contributor.author	Verbunt, F.	-
dc.contributor.author	Bhattacharya, D.	-
dc.contributor.author	Wijers, H.	-
dc.date.accessioned	2007-05-25T08:40:54Z	-
dc.date.available	2007-05-25T08:40:54Z	-
dc.date.issued	1996	-
dc.identifier.citation	IAU Colloquium, 1996, Vol.160, p47	en
dc.identifier.uri	http://hdl.handle.net/2289/2423	-
dc.description	Open Access. Pulsars: problems and progressAstronomical Society of the Pacific Conference Series, Vol. 105; Proceedings of the 160th colloquium of the International Astronomical Union held in Sydney; Australia; 8-12 January 1996; San Francisco: Astronomical Society of the Pacific (ASP); 1996; edited by S. Johnston, M.A. Walker, and M. Bailes.	en
dc.format.extent	161554 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of Pacific	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?1996ASPC..105...47H	en
dc.rights	1996 Astronomical Society of the Pacific	en
dc.title	The case for no field decay from improved pulsar population studies	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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