activity
20052026
most citedAn Ultraluminous X-ray Source Powered by An Accreting Neutron Star

767 citations · 5.6k across the 85 of their papers we have counts for

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Showing 2009Show all

11 papers · 1 filter

astro-ph.HE2009★ 169 cited

Black hole accretion disks in the canonical low-hard state

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

Stellar-mass black holes in the low-hard state may hold clues to jet formation and basic accretion disk physics, but the nature of the accretion flow remains uncertain. A standard…

astro-ph.HE2009★ 50 cited

On Neutral Absorption and Spectral Evolution in X-ray Binaries

J. M. Miller, E. M. Cackett, R. C. Reis

Current X-ray observatories make it possible to follow the evolution of transient and variable X-ray binaries across a broad range in luminosity and source behavior. In such studie…

astro-ph.HE2009★ 234 cited

Broad iron L-line and X-ray reverberation in 1H0707-495

A. Zoghbi, A. Fabian, P. Uttley +5

A detailed analysis of a long XMM-Newton observation of the Narrow Line Seyfert 1 galaxy 1H0707-495 is presented, including spectral fitting, spectral variability and timing studie…

astro-ph.HE2009★ 7 cited

Swift monitoring of Cygnus X-2: investigating the NUV-X-ray connection

E. S. Rykoff, E. M. Cackett, J. M. Miller

The neutron star X-ray binary (NSXRB) Cygnus X-2 was observed by the Swift satellite 51 times over a 4 month period in 2008 with the XRT, UVOT, and BAT instruments. During this cam…

astro-ph.HE2009★ 66 cited

Constraining the Spin of the Black Hole in Fairall 9 with Suzaku

S. Schmoll, J. M. Miller, M. Volonteri +6

We report on the results of spectral fits made to data obtained from a 168 ksec Suzaku observation of the Seyfert-1 galaxy Fairall 9. The source is clearly detected out to 30 keV.…

astro-ph.HE2009★ 185 cited

Relativistic Lines and Reflection from the Inner Accretion Disks Around Neutron Stars

E. M. Cackett, J. M. Miller, D. R. Ballantyne +6

A number of neutron star low-mass X-ray binaries have recently been discovered to show broad, asymmetric Fe K emission lines in their X-ray spectra. These lines are generally thoug…