Spectral properties of the X-ray binary pulsar LMC X-4 during different intensity states

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DC Field	Value	Language
dc.contributor.author	Naik, S.	-
dc.contributor.author	Paul, Biswajit	-
dc.date.accessioned	2012-07-17T04:28:56Z	-
dc.date.available	2012-07-17T04:28:56Z	-
dc.date.issued	2002-06	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 23, p27	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/4959	-
dc.description	Open Access	en
dc.description.abstract	We present spectral variations of the binary X-ray pulsar LMC X-4 observed with the RXTE/PCA during different phases of its 30.5 day long third period. Only out-of-eclipse data were used for this study. The 3-25 keV spectrum, modeled with high energy cut-off power-law and iron line emission is found to show strong dependence on the intensity state. Correlations between the Fe line emission flux and different parameters of the continuum are presented here.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2002JApA...23...27N	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/0211558	en
dc.relation.uri	http://dx.doi.org/10.1007/BF02702461	en
dc.rights	2002 Indian Academy of Sciences, Bangalore, India	en
dc.title	Spectral properties of the X-ray binary pulsar LMC X-4 during different intensity states	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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