Observational aspects of outbursting black hole sources: Evolution of spectro-temporal features and X-ray variability

被引:15
作者
Sreehari, H. [1 ,2 ]
Nandi, Anuj [1 ]
Radhika, D. [3 ]
Iyer, Nirmal [4 ]
Mandal, Samir [5 ]
机构
[1] ISRO Satellite Ctr, Space Astron Grp, ISITE Campus,Outer Ring Rd, Marathahalli 560037, Bengaluru, India
[2] Indian Inst Sci, Dept Phys, Bengaluru 560012, India
[3] Dayananda Sagar Univ, Dept Phys, Bengaluru 560068, India
[4] KTH PAP, Albanova Univ Ctr, S-10691 Stockholm, Sweden
[5] Indian Inst Space Sci & Technol, Dept Phys, Thiruvananthapuram 695547, Kerala, India
关键词
Accretion; X-ray binaries; black holes; ISM: jets and outflows; radiation mechanisms; QUASI-PERIODIC OSCILLATIONS; SPECTRAL PROPERTIES; IGR J17091-3624; FREQUENCY; GRO-J1655-40; FLOWS; MODEL; QPOS;
D O I
10.1007/s12036-018-9510-0
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on our attempt to understand the outbursting profile of Galactic Black Hole sources, keeping in mind the evolution of temporal and spectral features during the outburst. We present results of evolution of quasi-periodic oscillations, spectral states and possible connection with jet ejections during the outburst phase. Further, we attempt to connect the observedX-ray variabilities (i.e., 'class'/'structured' variabilities, similar to GRS 1915+105) with spectral states of black hole sources. Towards these studies, we consider three black hole sources that have undergone single (XTE J1859+226), a few (IGR J17091-3624) and many (GX 339-4) outbursts since the start of RXTE era. Finally, we model the broadband energy spectra (3-150 keV) of different spectral states using RXTE and NuSTAR observations. Results are discussed in the context of two-component advective flow model, while constraining the mass of the three black hole sources.
引用
收藏
页数:14
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