no code implementations • 29 Nov 2020 • Reimar Leike, Silvia Celli, Alberto Krone-Martins, Celine Boehm, Martin Glatzle, Yasou Fukui, Hidetoshi Sano, Gavin Rowell
Finally, using the fact that the supernova remnant is expected to be located in a dusty environment and that there appears to be only one such structure in the vicinity of RX J1713. 7-3946, we set a very precise constrain to the supernova remnant distance, at ($1. 12 \pm 0. 01$) kpc.
High Energy Astrophysical Phenomena Astrophysics of Galaxies Computational Physics Data Analysis, Statistics and Probability Applications
no code implementations • 28 Oct 2020 • Miranda Yew, Miroslav D. Filipović, Milorad Stupar, Sean D. Points, Manami Sasaki, Pierre Maggi, Frank Haberl, Patrick J. Kavanagh, Quentin A. Parker, Evan J. Crawford, Branislav Vukotić, Dejan Urošević, Hidetoshi Sano, Ivo R. Seitenzahl, Gavin Rowell, Denis Leahy, Luke M. Bozzetto, Chandreyee Maitra, Howard Leverenz, Jeffrey L. Payne, Laurence A. F. Park, Rami Z. E. Alsaberi, Thomas G. Pannuti
We present a new optical sample of three Supernova Remnants and 16 Supernova Remnant (SNR) candidates in the Large Magellanic Cloud(LMC).
High Energy Astrophysical Phenomena Astrophysics of Galaxies
