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20022009
most citedAdvection/Diffusion of Large-Scale B-Field in Accretion Disks

94 citations · 121 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2009★ 94 cited

Advection/Diffusion of Large-Scale B-Field in Accretion Disks

R. V. E. Lovelace, D. M. Rothstein, G. S. Bisnovatyi-Kogan

Activity of the nuclei of galaxies and stellar mass systems involving disk accretion to black holes is thought to be due to (1) a small-scale turbulent magnetic field in the disk (…

astro-ph.HE2009★ 10 cited

QPO Frequency - Color Radius Connection in GRS 1915+105: a Possible Turnover supporting AEI predictions

Valerie J. Mikles, Peggy Varniere, Stephen S. Eikenberry +2

It is widely believed that the low frequency quasi-periodic X-ray oscillations observed in microquasars are correlated to, but do not originate at, the physical radius of the inner…

astro-ph2007★ 8 cited

HST/NICMOS Observations of Fast Infrared Flickering in the Microquasar GRS 1915+105

Stephen S. Eikenberry, Shannon G. Patel, David M. Rothstein +3

We report infrared observations of the microquasar GRS 1915+105 using the NICMOS instrument of the Hubble Space Telescope during 9 visits in April-June 2003. During epochs of high…

astro-ph2006

Simulations of the Disk-Jet Interaction in GRS 1915+105 and Other Systems

David M. Rothstein

After an X-ray binary experiences a transient jet ejection, it undergoes a phase in which its X-ray light curve is dominated, for some time, by thermal emission from an accretion d…

astro-ph2005★ 9 cited

Does Low Frequency X-ray QPO Behavior in GRS 1915+105 Influence Subsequent X-ray and Infrared Evolution?

V. J. Mikles, S. S. Eikenberry, D. M. Rothstein

Using observations with the Rossi X-ray Timing Explorer, we examine the behavior of 2-10 Hz quasi-periodic oscillations (QPOs) during spectrally-hard dips in the x-ray light curve…

astro-ph2005

Observations of Rapid Disk-Jet Interaction in GRS 1915+105

David M. Rothstein, Stephen S. Eikenberry, Keith Matthews

We present evidence that ~ 30 minute episodes of jet formation in GRS 1915+105 may sometimes be a superposition of smaller, faster phenomena. Based on observations in 2002 July usi…