28 citations · 127 across the 9 of their papers we have counts for
9 papers
Two shell- and wing-shaped supernova remnants. Investigating the molecular environments around VRO 42.05.01 and G 350.0-2.0
Maria Arias, Ping Zhou, Alexandros Chiotellis +6
Supernova remnants (SNRs) are profoundly affected by their ambient medium. We present carbon monoxide (CO) observations around two mixed morphology SNRs, VRO 42.05.01 and G 350.0-2…
Detection of optical emission from the supernova remnant G7.7-3.7
V. Domček, J. V. Hernández Santisteban, A. Chiotellis +6
We present the first optical study of the supernova remnant (SNR) G7.7-3.7, with the aim of determining its evolutionary phase since it has been suggested to be the remnant of SN 3…
Multi-epoch properties of the warm absorber in the Seyfert 1 galaxy NGC 985
J. Ebrero, V. Domcek, G. A. Kriss +1
(Abridged) NGC 985 was observed by XMM-Newton twice in 2015, revealing that the source was coming out from a soft X-ray obscuration event that took place in 2013. These kinds of ev…
Unveiling pure-metal ejecta X-ray emission in supernova remnants through their radiative recombination continuum
Emanuele Greco, Jacco Vink, Marco Miceli +5
Spectral analysis of X-ray emission from ejecta in supernova remnants (SNRs) is hampered by the low spectral resolution of CCD cameras, which creates a degeneracy between the best-…
The environment of supernova remnant VRO 42.05.01 as probed with IRAM 30m molecular line observations
Maria Arias, Vladimir Domcek, Ping Zhou +1
The environment of supernova remnants (SNRs) is a key factor in their evolution, particularly at later stages of their existence. It is often assumed that mixed-morphology (MM) SNR…
Steep X-ray reflection emissivity profiles in AGN as the result of radially-structured disc ionisation
E. S. Kammoun, V. Domcek, J. Svoboda +2
X-ray observations suggest high compactness of coronae in active galactic nuclei as well as in X-ray binaries. The compactness of the source implies a strong radial dependence in t…