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20032005
most citedSimulating the Early Evolution of the Hard X-Ray Properties of a Young Stellar Population

2 citations · 2 across the 5 of their papers we have counts for

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astro-ph2005

Observational Signature of Tidal Disruption of a Star by a Massive Black Hole

Tamara Bogdanovic, Michael Eracleous, Suvrath Mahadevan +2

We have modeled the time-variable profiles of the Balmer alpha emission from the nonaxisymmetric disk and debris tail created in the tidal disruption of a solar-type star by a mill…

astro-ph2004

Non-stationary variability in AGN: the case of 3C 390.3

M. Gliozzi, I. E. Papadakis, R. M. Sambruna +1

We use data from a two-year intensive RXTE monitoring campaign of the broad-line radio galaxy 3C 390.3 to investigate its stationarity. In order to exploit the potential informatio…

astro-ph2003

Active Galaxies With Double-Peaked Emission Lines and What They Imply About the "Broad-Line Region"

Michael Eracleous

I review the distinguishing observational characteristics of active galaxies with double-peaked emission lines and their implications for the nature of the line-emitting region. Si…

astro-ph2003

Long Term Profile Variability of Double-Peaked Emission Lines in AGNs

Karen T. Lewis, Michael Eracleous, Jules P. Halpern +1

An increasing number of AGNs exhibit broad, double-peaked Balmer emission lines, which are thought to arise from the outer regions of the accretion disk which fuels the AGN. The li…

astro-ph20032 cited

Simulating the Early Evolution of the Hard X-Ray Properties of a Young Stellar Population

M. S. Sipior, M. Eracleous, S. Sigurdsson

We present an X-ray binary population synthesis model, and use it to simulate the evolution of X-ray binaries formed in a burst of star formation of duration 20 Myr and star-format…