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20012009
most citedRelativistic X-ray Lines from the Inner Accretion Disks Around Black Holes

409 citations · 1.2k across the 14 of their papers we have counts for

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astro-ph.HE20093 cited

The detection of Broad Iron K and L line emission in the Narrow-Line Seyfert 1 Galaxy 1H0707-495 using XMM-Newton

A. C. Fabian, A. Zoghbi, R. R. Ross +14

Since the discovery of the first broad iron-K line in 1995 from the Seyfert Galaxy MCG--6-30-15, broad iron-K lines have been found in several other Seyfert galaxies, from accretin…

astro-ph.HE20093 cited

Spin and Relativistic Phenomena Around Black Holes

L. Brenneman, J. M. Miller, K. Nandra +13

Since the seminal work of Penrose (1969) and Blandford & Znajek (1977), it has been realized that black hole spin may be an important energy source in astrophysics. The radio-loud/…

astro-ph.HE20092 cited

Fundamental Accretion and Ejection Astrophysics

J. M. Miller, M. Nowak, K. Nandra +11

Disk accretion may be the fundamental astrophysical process. Stars and planets form through the accretion of gas in a disk. Black holes and galaxies co-evolve through efficient dis…

astro-ph.HE20093 cited

Stellar-Mass Black Holes and Their Progenitors

J. M. Miller, P. Uttley, K. Nandra +14

If a black hole has a low spin value, it must double its mass to reach a high spin parameter. Although this is easily accomplished through mergers or accretion in the case of super…

astro-ph.HE200929 cited

Thermal emission from the stellar-mass black hole binary XTE J1118+480 in the low/hard state

R. C. Reis, J. M. Miller, A. C. Fabian

We report on the detection of a thermal-disk component from the stellar-mass black hole binary XTE J1118+480 in the canonical low/hard state. The presence of a thermal component wi…