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Thin Circular Disk Shells of OH Masers Toward SNRs
Published online by Cambridge University Press: 19 July 2016
Abstract
We propose a new model of distinct thin circular disk shells to analyze Gaussian fits to spectral features of OH emission at 1720 MHz toward supernova remnants. We have inferred that the OH(1720 MHz) maser features toward G348.5+0.1 are radiated from three distinct thin circular disk shells, and have obtained the parameters of the shells.
- Type
- Part 2: Supernova Remnants
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- Copyright © Astronomical Society of the Pacific 2004