activity
19982006
most citedProbing Quasar Outflows with Intrinsic Narrow Absorption Lines

1 citations · 1 across the 6 of their papers we have counts for

collaborators

11 papers

astro-ph20061 cited

Probing Quasar Outflows with Intrinsic Narrow Absorption Lines

T. Misawa, M. Eracleous, J. C. Charlton +5

We present statistical and monitoring results of narrow absorption lines that are physically related to quasars (i.e., intrinsic NALs). We use Keck/HIRES spectra of 37 optically br…

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-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-ph2002

Feeding the active nucleus of NGC 1097

Thaisa Storchi-Bergmann, Rodrigo Nemmen da Silva, Michael Eracleous

We discuss the signatures of an evolving accretion disk around the nucleus of NGC 1097, based on observations of its double-peaked H-alpha emission-line profile which cover a time…

astro-ph2002

Evolution of the accretion disk in the nucleus of NGC 1097

T. Storchi-Bergmann, R. Nemmen da Silva, M. Eracleous

We discuss the long-term evolution of the broad double-peaked H alpha profile of the LINER/Seyfert 1 nucleus of NGC 1097. Besides the previously known variation of the relative int…