no code implementations • 26 Jan 2021 • Naslim Neelamkodan, Kazuki Tokuda, Susmita Barman, Hiroshi Kondo, Hidetoshi Sano, Toshikazu Onishi
We determine the collision timescale $\sim$ 0. 2 Myr using the relative velocity ($\sim$ 5. 1 km s$^{-1}$) and displacement ($\sim$ 1. 1 pc) of those interacting filaments.
Astrophysics of Galaxies
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 • 6 Nov 2020 • Aya Bamba, Eri Watanabe, Koji Mori, Shinpei Shibata, Yukikatsu Terada, Hidetoshi Sano, Miroslav D. Filipovic
Depending on the emission models, the 3sigma upper-limit on the intrinsic 0. 5-7 keV flux to (2. 2-10. 0)e-14 erg/s/cm2.
High Energy Astrophysical Phenomena
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
no code implementations • 8 May 2020 • Kisetsu Tsuge, Kengo Tachihara, Yasuo Fukui, Hidetoshi Sano, Kazuki Tokuda, Junko Ueda, Daisuke Iono
Tsuge et al. (2020) showed that the five giant molecular complexes in the Antennae Galaxies have signatures of cloud-cloud collisions based on the ALMA archival data at 60 pc resolution.
Astrophysics of Galaxies
