activity
20002009
most citedLooking Into the Fireball: ROTSE-III and Swift Observations of Early GRB Afterglows

111 citations · 271 across the 5 of their papers we have counts for

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10 papers · 1 filter

astro-ph2008★ 38 cited

On the plasma temperature in supernova remnants with cosmic-ray modified shocks

L. O'C. Drury, F. A. Aharonian, D. Malyshev +1

Context: Multiwavelength observations of supernova remnants can be explained within the framework of the diffusive shock acceleration theory, which allows effective conversion of t…

astro-ph2007★ 83 cited

Variable VHE gamma-ray emission from non-blazar AGNs

F. M. Rieger, F. A. Aharonian

The observation of rapidly variable very high energy (VHE) gamma-rays from non-aligned active galactic nuclei (AGNs), as reported from M87, proves challenging for conventional theo…

astro-ph2005

Optical Lightcurve & Cooling Break of GRB 050502A

S. A. Yost, K. Alatalo, E. S. Rykoff +29

We present lightcurves of the afterglow of GRB050502A, including very early data at t-t_{GRB} < 60s. The lightcurve is composed of unfiltered ROTSE-IIIb optical observations from 4…

astro-ph2005

Broad-band electromagnetic radiation from microquasars interacting with ISM

V. Bosch-Ramon, F. A. Aharonian, J. M. Paredes

Microquasars (MQs) are galactic objects with relativistic jets that constitute a source population which can be responsible for production of a non-negligible fraction of the obser…

astro-ph2005

On the formation of energy spectra of synchrotron X-rays and inverse Compton gamma-rays in binary systems with luminous optical stars

D. Khangulyan, F. Aharonian

In this paper we study formation broad band energy spectra of electrons due to synchrotron radiation and inverse Compton (IC) scattering. The effect of transition of IC cooling fro…

astro-ph2004

Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM

V. Bosch-Ramon, F. A. Aharonian, J. M. Paredes

Microquasars are potential candidates to produce a non-negligible fraction of the observed galactic cosmic rays. The protons accelerated at the jet termination shock interact with…