Showing 21–40 of 57 results
/ Date/ Name
Dec 5, 2002Iron-Rich Ejecta in the Supernova Remnant DEM L71May 20, 2003An X-Ray Pulsar in the Oxygen-Rich Supernova Remnant G292.0+1.8Aug 19, 2004A Chandra ACIS view of the Thermal Composite Supernova Remnant 3C391Sep 18, 2002Revealing New Physical Structures in the Supernova Remnant N63A through Chandra Imaging SpectroscopyFeb 8, 2012Elemental Abundances in the Possible Type Ia Supernova Remnant G344.7-0.1Dec 3, 2001The Structure of the Oxygen-rich Supernova Remnant G292.0+1.8 from Chandra X-ray Images: Shocked Ejecta and Circumstellar MediumJun 4, 2001A Pulsar Wind Nebula in the Oxygen-Rich Supernova Remnant G292.0+1.8Aug 6, 2015The Properties of the Progenitor Supernova, Pulsar Wind, and Neutron Star inside PWN G54.1+0.3Aug 30, 2001Discovery of X-ray Pulsations from the Compact Central Source in the Supernova Remnant 3C 58Oct 26, 1999Nucleosynthesis and Mixing in Cassiopeia AMay 2, 2005Highly Clumpy Structure of the Thermal Composite Supernova Remnant 3C391 Unveiled by ChandraOct 15, 2007A Half-Megasecond Chandra Observation of the Oxygen-Rich Supernova Remnant G292.0+1.8Feb 27, 2016The Refined Shock Velocity of the X-Ray Filaments in the RCW 86 Northeast RimApr 2, 2007The Radio Emission, X-ray Emission, and Hydrodynamics of G328.4+0.2: A Comprehensive Analysis of a Luminous Pulsar Wind Nebula, its Neutron Star, and the Progenitor Supernova ExplosionJan 21, 1998Study of the Composite Supernova Remnant MSH 11-62Dec 29, 2003Nucleosynthesis in The Oxygen-Rich Supernova Remnant G292.0+1.8 from Chandra X-Ray SpectroscopyFeb 26, 2013Serendipitous Discovery of An Infrared Bow Shock Near PSR J1549-4848 with SpitzerSep 11, 2013A Chandra View Of Nonthermal Emission In The Northwestern Region Of Supernova Remnant RCW 86: Particle Acceleration And Magnetic FieldsJun 9, 2014Asymmetry in The Observed Metal-Rich Ejecta of Galactic Type Ia Supernova Remnant G299.2-2.9Jan 22, 2010The Outer Shock of the Oxygen-Rich Supernova Remnant G292.0+1.8: Evidence for the Interaction with the Stellar Winds from its Massive Progenitor