ON THE PROSPECT OF CONSTRAINING BLACK HOLE SPIN THROUGH X-RAY SPECTROSCOPY OF HOTSPOTS
Future X-ray instrumentation is expected to allow us to significantly improve the constraints derived from the Fe K lines in active galactic nuclei, such as the black hole angular momentum (spin) and the inclination angle of the putative accretion disk. We consider the possibility that measurements...
Main Authors: | Yaqoob, Tahir (Author), Karas, Vladimir (Author), Dovciak, Michal (Author), Murphy, Kendrah Dawn (Contributor) |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2015-03-16T14:26:53Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
BEYOND THE STANDARD MODEL OF THE DISC–LINE SPECTRAL PROFILES FROM BLACK HOLE ACCRETION DISCS
by: Vjaceslav Sochora, et al.
Published: (2014-08-01) -
X-ray spectroscopy of accreting black holes
by: Plant, Daniel
Published: (2014) -
Determining the spin of the Black Hole in the Active Galactic Nucleus NGC-4395 using X-Ray spectroscopy
by: Weimer, Celine, et al.
Published: (2013) -
X-ray reflection spectroscopy with Kaluza–Klein black holes
by: Jiachen Zhu, et al.
Published: (2020-07-01) -
Recoiling black holes: prospects for detection and implications of spin alignment
by: Blecha, Laura, et al.
Published: (2017)