Power spectrum analysis of the timing noise in 18 southern pulsars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1122

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DC Field	Value	Language
dc.contributor.author	D'Alessandro, F.	-
dc.contributor.author	Deshpande, A.A.	-
dc.contributor.author	McCulloch, P.M.	-
dc.date.accessioned	2006-01-09T05:55:41Z	-
dc.date.available	2006-01-09T05:55:41Z	-
dc.date.issued	1997	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1997, Vol.18, p5-14.	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/1122	-
dc.description.abstract	Power spectra of the timing noise observed in 18 southern pulsars have been derived using a novel technique, based on the CLEAN algorithm. Most of the spectra are well described by a single- or double- component power-law model. Some of these spectra can be interpreted in the context of one or more of the current timing noise models. The results combined with those obtained from the time-domain analyses of the timing activity in these pulsars are used to assess the viability of the various theoretical models of pulsar timing noise.	en
dc.format.extent	1666331 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: timing noise;	en
dc.subject	power spectra;	en
dc.subject	neutron star;	en
dc.title	Power spectrum analysis of the timing noise in 18 southern pulsars	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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