Showing 1–20 of 102 results
/ Date/ Name
Oct 1, 2004XMM-Newton Observations of G32.45+0.1and G38.55+0.0: diffuse hard X-ray sources found with the ASCA Galactic Plane SurveyFeb 8, 2012New Insights into SNR Evolution Revealed by the Discovery of Recombining PlasmasFeb 8, 2012Suzaku View of the Supernova Remnant RCW 86: X-Ray Studies of Newly-Discovered Fe-Rich EjectaAug 26, 2008Suzaku Observation of 30Dor C: A Supernova Remnant with the Largest Non-Thermal ShellSep 20, 2007Suzaku Observation of the RCW86 Northeastern ShellFeb 8, 2012Elemental Abundances in the Possible Type Ia Supernova Remnant G344.7-0.1Feb 14, 2015A Chandrasekhar Mass Progenitor for the Type Ia Supernova Remnant 3C 397 from The Enhanced Abundances of Nickel and ManganeseSep 21, 2009Discovery of Strong Radiative Recombination Continua from The Supernova Remnant IC 443 with SuzakuFeb 20, 2009Suzaku Spectroscopy of Vela Shrapnel BNov 18, 2016The Origin of the Iron-Rich Knot in Tycho's Supernova RemnantFeb 27, 2016The Refined Shock Velocity of the X-Ray Filaments in the RCW 86 Northeast RimJun 28, 2007X-Ray Spectroscopy of SN 1006 with SuzakuNov 11, 2018Evidence for Rapid Adiabatic Cooling as an Origin of the Recombining Plasma in the Supernova Remnant W49B Revealed by NuSTAR ObservationsMar 13, 2021Discovery of Double-Ring Structure in the Supernova Remnant N103B: Evidence for Bipolar Winds from a Type Ia Supernova ProgenitorMar 20, 2014Discriminating the Progenitor Type of Supernova Remnants with Iron K-Shell EmissionOct 31, 2013New Evidence for Efficient Collisionless Heating of Electrons at the Reverse Shock of a Young Supernova RemnantAug 26, 2024The XRISM First Light Observation: Velocity Structure and Thermal Properties of the Supernova Remnant N132DMar 17, 2020Uniform distribution of the extremely overionized plasma associated with the supernova remnant G359.1-0.5Jan 8, 2020A Nucleosynthetic Origin for the Southwestern Fe-rich Structure in Kepler's Supernova RemnantSep 25, 2022Discovery of Year-Scale Time Variability from Thermal X-ray Emission in Tycho's Supernova Remnant