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19941998
most citedOptical Appearance of the Debris of a Star Disrupted by a Massive Black Hole

259 citations · 753 across the 14 of their papers we have counts for

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astro-ph1998★ 173 cited

Tidal disruption rates of stars in observed galaxies

D. Syer, A. Ulmer

We derive the rates of capture, Ndot, of main sequence turn off stars by the central massive black hole in a sample of galaxies from Magorrian et al. 1998. The disruption rates are…

astro-ph1997★ 2 cited

Tidal Disruption Eddington Envelopes around Massive Black Holes

Andrew Ulmer, Bohdan Paczynski, Jeremy Goodman

Optically-thick envelopes may form following the tidal disruption of a star by a massive black hole. Such envelopes would reprocess hard radiation from accretion close to the black…

astro-ph1997

Evolution of Thick Accretion Disks Produced by Tidal Disruption Events

Andrew Ulmer

Geometrically thick disks may form after tidal disruption events, and rapid accretion may lead to short flares followed by long-term, lower-level emission. Using a novel accretion…

astro-ph1997★ 32 cited

Revisiting the Modified Eddington Limit for Massive Stars

Andrew Ulmer, Edward L. Fitzpatrick

We have determined the location of the line-opacity modified Eddington limit for stars in the LMC using the most recent atmosphere models combined with a precise mapping to the HR…

astro-ph1997

Flares from the Tidal Disruption of Stars by Massive Black Holes

Andrew Ulmer

Tidal disruption flares are differentiated into two classes -- those which are sub-Eddington and those which radiate near the Eddington limit. Flares from black holes above ~2 x 10…

astro-ph1997★ 259 cited

Optical Appearance of the Debris of a Star Disrupted by a Massive Black Hole

Abraham Loeb, Andrew Ulmer

We show that the disruption of a star by a 10^6 solar mass black hole in a galactic nucleus could under favorable circumstances produce an optically-thick envelope that radiates wi…