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The deepest radio study of the pulsar wind nebula G21.5−0.9: still no evidence for the supernova shell

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MULTI-WAVELENGTH STUDY OF THE SUPERNOVA REMNANT KES 79 (G33.6+0.1): ON ITS SUPERNOVA PROPERTIES AND EXPANSION INTO A MOLECULAR ENVIRONMENT

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MODELING THE X-RAYS FROM THE CENTRAL COMPACT OBJECT PSR J1852+0040 IN KESTEVEN 79: EVIDENCE FOR A STRONGLY MAGNETIZED NEUTRON STAR

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THE METAL-ENRICHED THERMAL COMPOSITE SUPERNOVA REMNANT KESTEVEN 41 (G337.8-0.1) IN A MOLECULAR ENVIRONMENT

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Fe-RICH EJECTA IN THE SUPERNOVA REMNANT G352.7–0.1 WITHSUZAKU

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Thermal luminosities of cooling neutron stars

A Y Potekhin, D A Zyuzin, D G Yakovlev, M V Beznogov and Yu A Shibanov
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FERMI-LAT OBSERVATIONS OF SUPERNOVA REMNANTS KESTEVEN 79

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DISCRIMINATING THE PROGENITOR TYPE OF SUPERNOVA REMNANTS WITH IRON K-SHELL EMISSION

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XMM-NEWTONANDCHANDRAOBSERVATIONS OF THE EJECTA-DOMINATED MIXED-MORPHOLOGY GALACTIC SUPERNOVA REMNANT G352.7–0.1

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Diffusion Ionised Gas in the Directions of the Supernova Remnant Kes 79 and Pulsar B1849+00

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THE FIRST FERMI LAT SUPERNOVA REMNANT CATALOG

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Discovery of Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Kesteven 79

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Evolving supernova remnants in multiphase interstellar media

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Chandrasekhar and Sub-Chandrasekhar Models for the X-Ray Emission of Type Ia Supernova Remnants. I. Bulk Properties

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DISCOVERY OF THE TRANSIENT MAGNETAR 3XMM J185246.6+003317 NEAR SUPERNOVA REMNANT KESTEVEN 79 WITH XMM-NEWTON

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CHASING THE IDENTIFICATION OF ASCA GALACTIC OBJECTS (ChIcAGO): AN X-RAY SURVEY OF UNIDENTIFIED SOURCES IN THE GALACTIC PLANE. I. SOURCE SAMPLE AND INITIAL RESULTS

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