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

Xiao, G.; Ji, L.; Staubert, R.; Ge, M.; Zhang, S.; Zhang, S.; Santangelo, A.; Ducci, L.; Liao, J.; Guo, C.; Li, X.; Zhang, W.; Qu, J.; Lu, F.; Li, T.; Song, L.; Xu, Y.; Bu, Q.; Cai, C.; Cao, X.; Chang, Z.; Chen, G.; Chen, L.; Chen, T.; Chen, Y.; Chen, Y.; Chen, Y.; Cui, W.; Cui, W.; Deng, J.; Dong, Y.; Du, Y.; Fu, M.; Gao, G.; Gao, H.; Gao, M.; Gu, Y.; Guan, J.; Gungor, Can; Han, D.; Huang, Y.; Huo, J.; Jia, S.; Jiang, L.; Jiang, W.; Jin, J.; Kong, L.; Li, B.; Li, C.; Li, G.; Li, M.; Li, W.; Li, X.; Li, X.; Li, Y.; Li, Z.; Liang, X.; Liu, C.; Li, G.; Liu, H.; Liu, X.; Liu, Y.; Lu, B.; Lu, X.; Luo, Q.; Luo, T.; Ma, X.; Meng, B.; Nang, Y.; Nie, J.; Qu, G.; Sai, N.; Song, S.; Sun, L.; Tan, Y.; Tao, L.; Tuo, Y.; Wang, C.; Wang, G.; Wang, J.; Wang, W.; Wang, Y.; Wen, X.; Wu, B.; Wu, B.; Wu, M.; Xiong, S.; Yang, J.; Yang, S.; Yang, Y.; Yin, Q.; Yin, Q.; Zhang, A.; Zhang, C.; Zhang, F.; Zhang, H.; Zhang, J.; Zhang, T.; Zhang, W.; Zhang, W.; Zhang, Y.; Zhang, Y.; Zhang, Y.; Zhang, Z.; Zhang, Z.; Zhao, H.; Zhao, X.; Zheng, S.; Zhou, J.; Zhu, Y.; Zhu, Y.

doi:10.1016/j.jheap.2019.09.002

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

Atıf İçin Kopyala

Xiao G. C., Ji L., Staubert R., Ge M. Y., Zhang S., Zhang S. N., ...Daha Fazla

JOURNAL OF HIGH ENERGY ASTROPHYSICS, cilt.23, ss.29-32, 2019 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 23
Basım Tarihi: 2019
Doi Numarası: 10.1016/j.jheap.2019.09.002
Dergi Adı: JOURNAL OF HIGH ENERGY ASTROPHYSICS
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Sayfa Sayıları: ss.29-32
İstanbul Üniversitesi Adresli: Hayır

Özet

The 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.