141 citations · 435 across the 23 of their papers we have counts for
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Simulated non-thermal emission from SNR G1.9+0.3
Marco A. Villagran, D. O. Gómez, P. F. Velázquez +7
Supernova remnants are the nebular leftover of defunct stellar environments, resulting from the interaction between a supernova blastwave and the circumstellar medium shaped by the…
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…
Deep optical study of the mixed-morphology supernova remnant G 132.7+1.3 (HB3)
P. Boumis, A. Chiotellis, V. Fragkou +8
We present optical ccd images of the large supernova remnant (SNR) G132.71.3 (HB3) covering its full extent for the first time, in the emission lines of H[N II], [S II] and…
VRO 42.05.01: A supernova remnant resulted by a supersonic, mass losing progenitor star
A. Chiotellis, P. Boumis, S. Derlopa +1
We present a model for the Galactic supernova remnant (SNR) VRO 42.05.01, suggesting that its intriguing morphology can be explained by a progenitor model of a supersonically movin…
The imprint of a symbiotic binary progenitor on the properties of Kepler's supernova remnant
A. Chiotellis, K. M. Schure, Jacco Vink
We present a model for the Type Ia supernova remnant (SNR) of SN 1604, also known as Kepler's SNR. We find that its main features can be explained by a progenitor model of a symbio…