Published August 1, 1975 | Version v1
Journal article

X-ray structure of the Vela supernova remnant

  • 1. California Institute of Technology, Pasadena

Description

The X-ray surface brightness distribution of the Vela supernova remnant is presented in three energy intervals on scales of 1.0 deg2 and 0.44 deg2. The 0.15--1.0 keV X-ray emission exhibits two principal regions of enhancement and a general limb brightening which may imply a shell-like source structure

Additional details

Identifiers

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
199
Journal Issue
3
Series
Astrophys. J.
Journal Page Range
680
ISSN
0004-637X

Optional Information

Notes
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