activity
20052008
most citedOrbital X-Ray Variability of the Microquasar LS 5039

86 citations · 290 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph2008

The TeV emitter structure in LS 5039

Valenti Bosch-Ramon, Dmitry Khangulyan, Felix Aharonian

LS 5039 is an X-ray binary detected at very high energies. Along the orbit, there is a significant detection even during the superior conjunction of the compact object, when very l…

astro-ph20081 cited

Non-thermal emission from massive YSOs. Exploring the spectrum at high energies

Anabella T. Araudo, Gustavo E. Romero, Valenti Bosch-Ramon +1

Thermal radio and X-ray emission has been traditionally associated with the formation of stars. However, in recent years, non-thermal radiation from massive star forming regions ha…

astro-ph20082 cited

The physics of non-thermal radiation in microquasars

V. Bosch-Ramon

Microquasars are binary systems that harbor a normal star and a compact object (black-hole or neutron star), and show relativistic outflows (or jets). The matter that forms these j…

astro-ph200774 cited

Upper limit for gamma-ray emission above 140 GeV from the dwarf spheroidal galaxy Draco

MAGIC Collaboration, J. Albert

The nearby dwarf spheroidal galaxy Draco with its high mass to light ratio is one of the most auspicious targets for indirect dark matter searches. Annihilation of hypothetical DM…

astro-ph200754 cited

Leptonic secondary emission in a hadronic microquasar model

M. Orellana, P. Bordas, V. Bosch-Ramon +2

Context: It has been proposed that the origin of the very high-energy photons emitted from high-mass X-ray binaries with jet-like features, so-called microquasars (MQs), is related…

astro-ph200757 cited

Gamma-ray emission from massive young stellar objects

A. T. Araudo, G. E. Romero, V. Bosch-Ramon +1

Massive stars form in dense and massive molecular cores. The exact formation mechanism is unclear, but it is possible that some massive stars are formed by processes similar to tho…