activity
19962021
most citedRadio emission from Supernova Remnants

166 citations · 1.1k across the 42 of their papers we have counts for

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17 papers · 1 filter

astro-ph.GA2019★ 9 cited

Evolving Supernova Remnants in Multiphase Interstellar Media

Marco A. Villagran, P. F. Velázquez, D. O. Gómez +1

We performed three-dimensional magnetohydrodynamic simulations to study the evolution of a supernova remnant (SNR) in a turbulent neutral atomic interstellar medium. The media used…

astro-ph.GA2017★ 10 cited

Radio and X-ray properties of the source G29.37+0.1 linked to HESS J1844-030

G. Castelletti, L. Supan, A. Petriella +2

Using observations carried out with the GMRT, we performed high-quality full-synthesis imaging at 610 MHz of the source G29.37+0.1, which is an as-yet-unclassified object linked to…

astro-ph.GA2016★ 6 cited

HESS J1943+213: a non-classical high-frequency-peaked BL Lac object

Samayra M. Straal, Krisztina E. Gabanyi, Joeri van Leeuwen +5

HESS J1943+213 is an unidentified TeV source that is likely a high-frequency-peaked BL Lac (HBL) object but also compatible with a pulsar wind nebula (PWN) nature. Each of these en…

astro-ph.GA2015★ 4 cited

HII region G46.5-0.2: the interplay between ionizing radiation, molecular gas and star formation

S. Paron, M. E. Ortega, G. Dubner +8

HII regions are particularly interesting because they can generate dense layers of gas and dust, elongated columns or pillars of gas pointing towards the ionizing sources, and come…

astro-ph.GA2015★ 2 cited

e-MERLIN observations of the puzzling TeV source HESS J1943+213

K. E. Gabanyi, G. Dubner, E. Giacani +2

HESS J1943+213 is a TeV source close to the Galactic plane proposed to be a BL Lac object. Our high resolution EVN observation failed to recover two thirds of the source flux densi…

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…