output
20022026
most citedDark Matter Results from 225 Live Days of XENON100 Data

1.4k citations

Showing 2006 · astro-phShow all

48 papers · 2 filters

astro-ph2006

Forced oscillations in relativistic accretion disks and QPOs

J. Petri

In this work we explore the idea that the high frequency QPOs observed in LMXBs may be explained as a resonant coupling between the neutron star spin and epicyclic modes of accreti…

astro-ph2006★ 10 cited

Hemispherical transport equation: modeling of quasiparallel collisionless shocks

V. N. Zirakashvili

Using a so-called hemispherical model we derive a general transport equation for cosmic ray and thermal particles scattered in pitch angle by magnetic inhomogeneities in a moving c…

astro-ph2006★ 13 cited

A low density of the Extragalactic Background Light revealed by the H.E.S.S. spectra of the BLLac objects 1ES 1101-232 and H 2356-309

L. Costamante

The unexpectedly hard spectra measured by HESS for the BLLacs 1ES 1101-232 and H 2356-309 has allowed an upper limit on the Extragalactic Background Light (EBL) to be derived in th…

astro-ph2006★ 189 cited

H.E.S.S. observations of the supernova remnant RX J0852.0-4622: shell-type morphology and spectrum of a widely extended VHE gamma-ray source

HESS Collaboration, F. A. Aharonian

The shell-type supernova remnant RX J0852.0-4622 was observed with the High Energy Stereoscopic System (H.E.S.S.) of Atmospheric Cherenkov Telescopes between December 2004 and May…

astro-ph2006★ 14 cited

Theoretical overview on high-energy emission in microquasars

V. Bosch-Ramon

Microquasar (MQ) jets are sites of particle acceleration and synchrotron emission. Such synchrotron radiation has been detected coming from jet regions of different spatial scales,…

astro-ph2006★ 248 cited

Analytical solutions for energy spectra of electrons accelerated by nonrelativistic shock-waves in shell type supernova remnants

V. N. Zirakashvili, F. Aharonian

%context {Recent observations of hard X-rays and very high energy gamma-rays from a number of young shell type supernova remnants indicate the importance of detailed quantitative s…