output
19922026
Showing 2014 · astro-ph.HEShow all

68 papers · 2 filters

astro-ph.HE2014★ 25 cited

Internal shocks driven by accretion flow variability in the compact jet of the black hole binary GX 339-4

S. Drappeau, J. Malzac, J. Belmont +2

In recent years, compact jets have been playing a growing role in the understanding of accreting black hole engines. In the case of X-ray binary systems, compact jets are usually a…

astro-ph.HE2014★ 15 cited

The - relation and the internal shock model

R. Mochkovitch, L. Nava

The validity of the - correlation in gamma-ray bursts and the possibility of explaining the prompt emission with internal shocks are highly debated questi…

astro-ph.HE2014★ 30 cited

H.E.S.S. detection of TeV emission from the interaction region between the supernova remnant G349.7+0.2 and a molecular cloud

H. E. S. S. Collaboration, :, A. Abramowski +224

G349.7+0.2 is a young Galactic supernova remnant (SNR) located at the distance of 11.5 kpc and observed across the entire electromagnetic spectrum from radio to high energy (HE) Ga…

astro-ph.HE2014★ 63 cited

The X-ray Flux Distribution of Sagittarius A* as Seen by Chandra

J. Neilsen, S. Markoff, M. A. Nowak +11

We present a statistical analysis of the X-ray flux distribution of Sgr A* from the Chandra X-ray Observatory's 3 Ms Sgr A* X-ray Visionary Project (XVP) in 2012. Our analysis indi…

astro-ph.HE2014★ 8 cited

HI study of the environment around ESO 243-49, the host galaxy of an intermediate mass black hole

A. Musaeva, B. S. Koribalski, S. A. Farrell +9

The lenticular galaxy ESO 243-49 hosts the ultraluminous X-ray source HLX-1, the best candidate intermediate mass black hole (IMBH) currently known. The environments of IMBHs remai…

astro-ph.HE2014★ 18 cited

A Suzaku view of IGR J16393-4643

Nazma Islam, Chandreyee Maitra, Pragati Pradhan +1

The pulsar IGR J16393-4643 belongs to a class of highly absorbed supergiant HMXBs, characterised by very high column density of absorbing matter. We present the results of the simu…