用相对论 X 射线反射成分的测量探测黑洞引擎
高能天体物理现象
2019-03-19 v1
摘要
在过去的几十年里,X 射线光谱学已被证明是估计黑洞自旋以及数十个活动星系核和黑洞 X 射线双星中若干其他关键参数的有力工具。在本白皮书里,我们讨论在未来十年中探索、发现和研究天体物理黑洞所预期的观测与理论挑战。我们聚焦于吸积黑洞及其电磁特征,特别着重于其 X 射线光谱中相对论反射成分的测量。
引用
@article{arxiv.1903.07130,
title = {Probing the Black Hole Engine with Measurements of the Relativistic X-ray Reflection Component},
author = {Javier A. García and Matteo Bachetti and David R. Ballantyne and Laura Brenneman and Murray Brightman and Riley M. Connors and Thomas Dauser and Andrew Fabian and Felix Fuerst and Poshak Gandhi and Nikita Kamraj and Erin Kara and Kristin Madsen and Jon M. Miller and Michael Nowak and Michael L. Parker and Christopher Reynolds and James Steiner and Daniel Stern and Corbin Taylor and John Tomsick and Dominic Walton and Jörn Wilms and Abderahmen Zoghbi},
journal= {arXiv preprint arXiv:1903.07130},
year = {2019}
}
备注
Astro 2020 Decadal science White Paper