activity
19952014
most citedAdvection-Dominated Accretion and the Spectral States of Black Hole X-Ray Binaries: Application to Nova Muscae 1991

1.3k citations · 2.9k across the 19 of their papers we have counts for

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astro-ph2007★ 33 cited

Spitzer Space Telescope observations of magnetic cataclysmic variables: possibilities for the presence of dust in polars

C. S. Brinkworth, D. W. Hoard, S. Wachter +6

We present Spitzer Space Telescope photometry of six short-period polars, EF Eri, V347 Pav, VV Pup, V834 Cen, GG Leo, and MR Ser. We have combined the Spitzer Infrared Array Camera…

astro-ph2003★ 3 cited

Simultaneous optical and X-ray high speed photometry of Cyg X-2

G. Dubus, B. Kern, A. A. Esin +2

The X-ray emission from X-ray binaries may originate in flares occurring when magnetic loops anchored in the disc reconnect. In analogy with our Sun, H alpha emission should arise…

astro-ph2001★ 170 cited

Modeling the Low State Spectrum of the X-Ray Nova XTE J1118+480

A. A. Esin, J. E. McClintock, J. J. Drake +4

Based on recent multiwavelength observations of the new X-ray nova XTE J1118+480, we can place strong constraints on the geometry of the accretion flow in which a low/hard state sp…

astro-ph2000★ 501 cited

On The Synchrotron Self-Compton Emission from Relativistic Shocks and Its Implications for Gamma-Ray Burst Afterglows

Re'em Sari, Ann A. Esin

We consider the effects of inverse Compton scattering of synchrotron photons from relativistic electrons in GRB afterglows. We compute the spectrum of the inverse Compton emission…

astro-ph2000★ 80 cited

Dust Echos from Gamma Ray Bursts

Ann A. Esin, Roger Blandford

The deviation from the power-law decline of the optical flux observed in GRB 970228 and GRB 980326 has been used recently to argue in favor of the connection between GRBs and super…

astro-ph2000★ 3 cited

The 1996 outburst of GRO J1655-40: disc irradiation and enhanced mass transfer

A. A. Esin, J. -P. Lasota, R. I. Hynes

We show that the 1996 outburst of the X-ray binary transient system GRO J1655-40 can be explained by the standard dwarf-nova type disc instability, followed by an episode of enhanc…