Latest results of pulse phase resolved spectroscopy of cyclotron lines in accretion powered pulsars

We have performed pulse phase resolved spectroscopy of the Cyclotron Resonance Scattering Features (CRSF) of some bright accretion powered X-ray pulsars like 1A 1118-61, Vela X-1, A0535+26, XTE J1946+274, 4U 1907+09, 4U 1626-67 and GX 301-2 using Suzaku observations with long exposures. We have perf...

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Main Authors: Maitra Chandreyee, Paul Biswajit
Format: Article
Language:English
Published: EDP Sciences 2014-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20136406008
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author Maitra Chandreyee
Paul Biswajit
author_facet Maitra Chandreyee
Paul Biswajit
author_sort Maitra Chandreyee
collection DOAJ
description We have performed pulse phase resolved spectroscopy of the Cyclotron Resonance Scattering Features (CRSF) of some bright accretion powered X-ray pulsars like 1A 1118-61, Vela X-1, A0535+26, XTE J1946+274, 4U 1907+09, 4U 1626-67 and GX 301-2 using Suzaku observations with long exposures. We have performed the study using different spectral models for the continuum and have obtained similar patterns of variations of the CRSF in all the cases, thus demonstrating the robustness of our results. Pulse phase dependence of the CRSF in XTE J1946+274 has been obtained for the first time, and phase resolved variations of the CRSF in 4U 1907+09 has been compared at factor of ~ 2 difference in luminosity. We have also studied the pulse profiles of these objects near the CRSF energy, and have noticed an increased pulse fraction and/or a change in the pulse shape near the CRSF energy for some sources. The implications of the results are discussed.
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spelling doaj.art-733a2836b9d244b283b5431ee29dddf32022-12-21T21:09:05ZengEDP SciencesEPJ Web of Conferences2100-014X2014-01-01640600810.1051/epjconf/20136406008epjconf_mag2013_06008Latest results of pulse phase resolved spectroscopy of cyclotron lines in accretion powered pulsarsMaitra ChandreyeePaul Biswajit0Raman Research InstituteWe have performed pulse phase resolved spectroscopy of the Cyclotron Resonance Scattering Features (CRSF) of some bright accretion powered X-ray pulsars like 1A 1118-61, Vela X-1, A0535+26, XTE J1946+274, 4U 1907+09, 4U 1626-67 and GX 301-2 using Suzaku observations with long exposures. We have performed the study using different spectral models for the continuum and have obtained similar patterns of variations of the CRSF in all the cases, thus demonstrating the robustness of our results. Pulse phase dependence of the CRSF in XTE J1946+274 has been obtained for the first time, and phase resolved variations of the CRSF in 4U 1907+09 has been compared at factor of ~ 2 difference in luminosity. We have also studied the pulse profiles of these objects near the CRSF energy, and have noticed an increased pulse fraction and/or a change in the pulse shape near the CRSF energy for some sources. The implications of the results are discussed.http://dx.doi.org/10.1051/epjconf/20136406008
spellingShingle Maitra Chandreyee
Paul Biswajit
Latest results of pulse phase resolved spectroscopy of cyclotron lines in accretion powered pulsars
EPJ Web of Conferences
title Latest results of pulse phase resolved spectroscopy of cyclotron lines in accretion powered pulsars
title_full Latest results of pulse phase resolved spectroscopy of cyclotron lines in accretion powered pulsars
title_fullStr Latest results of pulse phase resolved spectroscopy of cyclotron lines in accretion powered pulsars
title_full_unstemmed Latest results of pulse phase resolved spectroscopy of cyclotron lines in accretion powered pulsars
title_short Latest results of pulse phase resolved spectroscopy of cyclotron lines in accretion powered pulsars
title_sort latest results of pulse phase resolved spectroscopy of cyclotron lines in accretion powered pulsars
url http://dx.doi.org/10.1051/epjconf/20136406008
work_keys_str_mv AT maitrachandreyee latestresultsofpulsephaseresolvedspectroscopyofcyclotronlinesinaccretionpoweredpulsars
AT paulbiswajit latestresultsofpulsephaseresolvedspectroscopyofcyclotronlinesinaccretionpoweredpulsars