Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7877
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dc.contributor.authorDevasia, Jincy-
dc.contributor.authorPaul, Biswajit-
dc.contributor.authorJames, Marykutty-
dc.contributor.authorIndulekha, K-
dc.date.accessioned2022-01-18T10:53:29Z-
dc.date.available2022-01-18T10:53:29Z-
dc.date.issued2011-02-
dc.identifier.citationProceedings of the 29th Annual Meeting of the Astronomical Society of India, Chhattisgarh, Febrauary 23-25, Vol.3, Edited by P. Khare and C.H. Ishwara-Chandra, 2011, p137en_US
dc.identifier.urihttp://hdl.handle.net/2289/7877-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en_US
dc.description.abstractWe report detection of sharp dips in the pulse profiles of several persistent and transient accretion powered X-ray pulsars using RXTE observations. The pulse profiles of accretion powered pulsars carry a lot of information regarding the radiative processes near the surface of the star, magnetic fields that channel the accretion flow etc. The dips in the pulse profiles can be due to the interaction of accretion column with the emitting radiation as it passes through the line of sight. We have also investigated the energy and intensity dependence and phase width of these dips to have a better understanding of the nature of the absorbing material. Any intensity dependence of the pulse phase of the dips will also reveal the nature of the absorbing structure in relation to the neutron staren_US
dc.language.isoenen_US
dc.publisherTIFR for the Astronomical Society of Indiaen_US
dc.relation.urihttps://ui.adsabs.harvard.edu/abs/2011ASInC...3..137D/abstracten_US
dc.rights2011 The Astronomical Society of Indiaen_US
dc.titleDips in the pulse profiles of accretion powered pulsarsen_US
dc.typeAbstracten_US
Appears in Collections:Research Papers (A&A)

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