activity
20012015
most citedXMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source

149 citations · 343 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2015★ 3 cited

The southern molecular environment of SNR G18.8+0.3

S. Paron, M. Celis Peña, M. E. Ortega +4

In a previous paper we have investigated the molecular environment towards the eastern border of the SNR G18.8+0.3. Continuing with the study of the surroundings of this SNR, in th…

astro-ph.GA2013★ 12 cited

A bright-rimmed cloud sculpted by the H ii region Sh2-48

M. E. Ortega, S. Paron, E. Giacani +2

To characterize a bright-rimmed cloud embedded in the HII region Sh2-48 searching for evidence of triggered star formation. We carried out observations towards a region of 2'x2' ce…

astro-ph.GA2012★ 14 cited

Outflowing activity in the UCHII region G045.47+0.05

M. E. Ortega, S. Paron, S. Cichowolski +2

Aims. This work aims at investigating the molecular gas in the surroundings of the ultra-compact HII region G045.47+0.05 looking for evidence of molecular outflows. Methods. We car…

astro-ph.HE2011★ 1 cited

Radio observations of Supernova Remnants and the surrounding molecular gas

G. Dubner

Supernova Remnants (SNRs) are believed to be the main source of Galactic cosmic rays (CR). The strong SNR shocks provide ideal acceleration sites for particles of at least 10^14 eV…

astro-ph.HE2009★ 74 cited

A joint spectro-imaging analysis of the XMM-Newton and HESS observations of the supernova remnant RX J1713.7-3946

F. Acero, J. Ballet, A. Decourchelle +5

The supernova remnant (SNR) RX J1713.7-3946 (also known as G347.3-0.5) is part of the class of remnants dominated by synchrotron emission in X-rays. It is also one of the few shell…

astro-ph2006★ 5 cited

On the nature of the hard X-ray source IGR J2018+4043

A. M. Bykov, A. M. Krassilchtchikov, Yu. A. Uvarov +13

We found a very likely counterpart to the recently discovered hard X-ray source IGR J2018+4043 in the multi-wavelength observations of the source field. The source, originally disc…