XMM-Newton observations of the supernova remnant IC 443

2008/04/07 by E. Troja, Eleonora Troja, F. Bocchino +5 · 1 citation
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Gamma-ray bursts and supernovae #Ionization #Near-Earth supernova #Nebula #Physics #Pulsar #Pulsar wind nebula #Stars #Supernova #Supernova remnant #astro-ph

paper · pdf · doi:10.1051/0004-6361:20079123

9 pages, 7 figures, accepted for publication in A&A. For hi-res figures, see http://www.astropa.unipa.it/Library/OAPA_preprints/aa20079123.pdf

arxiv created 2008/04/07 · openalex publication_date 2008/05/06 · arxiv updated 2009/12/01 · openalex created_date 2022/08/27 · openalex updated_date 2026/07/31

Abstract

Aims. We investigate the spatial distribution of the physical and chemical properties of the hot X-ray emitting plasma of the supernova remnant IC 443, to derive important constraints on its ionization stage, on the progenitor supernova explosion, on the age of the remnant, and its physical association with a close pulsar wind nebula.

Citations

• Collisional Plasma Models with APEC/APED: Emission-Line Diagnostics of Hydrogen-like and Helium-like Ions
• The X‐Ray Structure of the Pulsar Bow Shock G189.22+2.90 in the Supernova Remnant IC 443
• The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis
• Studying millisecond pulsars in X-rays
• The Evolution of Supernovae in Circumstellar Wind‐Blown Bubbles. I. Introduction and One‐Dimensional Calculations
• An evolutionary model for pulsar-driven supernova remnants
• The plerion nebula in IC 443: The XMM-Newton view
• XMM‐NewtonObservations of the Supernova Remnant IC 443. I. Soft X‐Ray Emission from Shocked Interstellar Medium

Cited by

• AKARINEAR-INFRARED SPECTRAL OBSERVATIONS OF SHOCKED H2GAS OF THE SUPERNOVA REMNANT IC 443