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VLBI Observations of SNR in M82 - Is 41.95+575 an Anomalous SNR or Something Else ?
Published online by Cambridge University Press: 13 May 2016
Abstract
Global VLBI 1.7GHz datasets from 1990 and 1998 have been used to study the evolution of SNR 41.95+575 in M82. An expansion velocity of around 1800 km/s is found with an implied birth around 1915. A young 41.95+575 would resemble radio supernovae seen in Arp220, although it could also be an evolving accretion disc system
- Type
- Supernovae, Pulsars, and the Interstellar Medium
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- Copyright © Astronomical Society of the Pacific 2001