no code implementations • 11 Feb 2021 • D. M. -A. Meyer, M. Pohl, M. Petrov, L. Oskinova
Our models are qualitatively consistent with the radio appearance of several remnants of high-mass progenitors, namely the bilateral G296. 5+10. 0 and the shell-type remnants CTB109 and Kes 17, respectively.
High Energy Astrophysical Phenomena Astrophysics of Galaxies Solar and Stellar Astrophysics
no code implementations • 22 Dec 2020 • M. Martínez-Chicharro, V. Grinberg, J. M. Torrejón, N. Schulz, L. Oskinova, M. Nowak, F. Fürst, N. Hell, R. Hainich
We present an analysis of the first observation of the iconic High Mass X-ray Binary \so with the \chandra High Energy Transmission Gratings during an X-ray eclipse.
High Energy Astrophysical Phenomena
