ASCA and XMM-Newton observations of the galactic supernova remnant G311.5−0.3

We present an analysis of X-ray observations made with ASCA and XMM-Newton of the Galactic supernova remnant (SNR) G311.5−0.3. Prior infrared and radio observations of this SNR have revealed a shell-like morphology at both wavelengths. The spectral index of the radio emission is consistent...

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Bibliographic Details
Main Authors: Pannuti T.G., Filipović M.D., Luken K., Wong G.F., Manojlović P., Maxted N., Roper Q.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2017-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2017/1450-698X1795023P.pdf