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Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations

dc.contributor.authorDeng, J. K.
dc.contributor.authorDucci, L.
dc.contributor.authorLiao, J. Y.
dc.contributor.authorGuo, C. C.
dc.contributor.authorLi, X. B.
dc.contributor.authorZhang, W.
dc.contributor.authorQu, J. L.
dc.contributor.authorLu, F. J.
dc.contributor.authorLi, T. P.
dc.contributor.authorSong, L. M.
dc.contributor.authorXiong, S. L.
dc.contributor.authorYang, J. W.
dc.contributor.authorYang, S.
dc.contributor.authorYang, Y. J.
dc.contributor.authorYin, Q. B.
dc.contributor.authorYin, Q. Q.
dc.contributor.authorZhang, A. M.
dc.contributor.authorZhang, C. M.
dc.contributor.authorZhang, F.
dc.contributor.authorZhang, H. M.
dc.contributor.authorZhang, J.
dc.contributor.authorZhang, T.
dc.contributor.authorZhang, W. C.
dc.contributor.authorZhang, W. Z.
dc.contributor.authorZhang, Y.
dc.contributor.authorZhang, Y. F.
dc.contributor.authorZhang, Y. J.
dc.contributor.authorZhang, Z.
dc.contributor.authorZhang, Z. L.
dc.contributor.authorZhao, H. S.
dc.contributor.authorZhao, X. F.
dc.contributor.authorZheng, S. J.
dc.contributor.authorZhou, J. F.
dc.contributor.authorZhu, Y.
dc.contributor.authorZhu, Y. X.
dc.contributor.authorGungor, C.
dc.contributor.authorXiao, G. C.
dc.contributor.authorJi, L.
dc.contributor.authorStaubert, R.
dc.contributor.authorGe, M. Y.
dc.contributor.authorZhang, S.
dc.contributor.authorZhang, S. N.
dc.contributor.authorXu, Y. P.
dc.contributor.authorBu, Q. C.
dc.contributor.authorCai, C.
dc.contributor.authorCao, X. L.
dc.contributor.authorChang, Z.
dc.contributor.authorChen, G.
dc.contributor.authorChen, L.
dc.contributor.authorChen, T. X.
dc.contributor.authorChen, Y. B.
dc.contributor.authorChen, Y.
dc.contributor.authorChen, Y. P.
dc.contributor.authorCui, W.
dc.contributor.authorCui, W. W.
dc.contributor.authorSantangelo, A.
dc.contributor.authorDong, Y. W.
dc.contributor.authorDu, Y. Y.
dc.contributor.authorFu, M. X.
dc.contributor.authorGao, G. H.
dc.contributor.authorGao, H.
dc.contributor.authorGao, M.
dc.contributor.authorGu, Y. D.
dc.contributor.authorGuan, J.
dc.contributor.authorHan, D. W.
dc.contributor.authorHuang, Y.
dc.contributor.authorHuo, J.
dc.contributor.authorJia, S. M.
dc.contributor.authorJiang, L. H.
dc.contributor.authorJiang, W. C.
dc.contributor.authorJin, J.
dc.contributor.authorKong, L. D.
dc.contributor.authorLi, B.
dc.contributor.authorLi, C. K.
dc.contributor.authorLi, G.
dc.contributor.authorLi, M. S.
dc.contributor.authorLi, W.
dc.contributor.authorLi, X.
dc.contributor.authorLi, X. F.
dc.contributor.authorLi, Y. G.
dc.contributor.authorLi, Z. W.
dc.contributor.authorLiang, X. H.
dc.contributor.authorLiu, C. Z.
dc.contributor.authorLi, G. Q.
dc.contributor.authorLiu, H. W.
dc.contributor.authorLiu, X. J.
dc.contributor.authorLiu, Y. N.
dc.contributor.authorLu, B.
dc.contributor.authorLu, X. F.
dc.contributor.authorLuo, Q.
dc.contributor.authorLuo, T.
dc.contributor.authorMa, X.
dc.contributor.authorMeng, B.
dc.contributor.authorNang, Y.
dc.contributor.authorNie, J. Y.
dc.contributor.authorQu, G.
dc.contributor.authorSai, N.
dc.contributor.authorSong, S. X.
dc.contributor.authorSun, L.
dc.contributor.authorTan, Y.
dc.contributor.authorTao, L.
dc.contributor.authorTuo, Y. L.
dc.contributor.authorWang, C.
dc.contributor.authorWang, G. F.
dc.contributor.authorWang, J.
dc.contributor.authorWang, W. S.
dc.contributor.authorWang, Y. S.
dc.contributor.authorWen, X. Y.
dc.contributor.authorWu, B. B.
dc.contributor.authorWu, B. Y.
dc.contributor.authorWu, M.
dc.date.accessioned2021-03-06T09:00:59Z
dc.date.available2021-03-06T09:00:59Z
dc.identifier.citationXiao G. C. , Ji L., Staubert R., Ge M. Y. , Zhang S., Zhang S. N. , Santangelo A., Ducci L., Liao J. Y. , Guo C. C. , et al., "Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations", JOURNAL OF HIGH ENERGY ASTROPHYSICS, cilt.23, ss.29-32, 2019
dc.identifier.issn2214-4048
dc.identifier.othervv_1032021
dc.identifier.otherav_e3ba00e1-76c2-4dde-964f-00b33100ec8a
dc.identifier.urihttp://hdl.handle.net/20.500.12627/149840
dc.identifier.urihttps://doi.org/10.1016/j.jheap.2019.09.002
dc.description.abstractThe long-term evolution of the centroid energy of the CRSF in Her X-1 is still a mystery. We report a new measurement from a campaign between Insight-HXMT and NuSTAR performed in February 2018. Generally, the two satellites show well consistent results of timing and spectral properties. The joint spectral analysis confirms that the previously observed long decay phase has ended, and that the line energy instead keeps constant around 37.5 keV after flux correction. (C) 2019 The Author(s). Published by Elsevier B.V.
dc.language.isoeng
dc.subjectFizik
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.titleConstant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations
dc.typeMakale
dc.relation.journalJOURNAL OF HIGH ENERGY ASTROPHYSICS
dc.contributor.departmentChinese Academy of Sciences , ,
dc.identifier.volume23
dc.identifier.startpage29
dc.identifier.endpage32
dc.contributor.firstauthorID105974


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