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Distinguishing Models for ACIS Data of Diffuse Emission
Published online by Cambridge University Press: 30 March 2016
Abstract
Discussed here is the issue of discriminating different spectral models for diffuse emission observations with the Chandra ACIS. First background models are considered. Then standard source models such as non-ionization equilibrium and ionization equilibrium models and models with different metal abundances are considered. The datasets used are from Chandra ACIS observations of diffuse emission, in particular of the Cygnus Loop supernova remnant.
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- I. Joint Discussions
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- Copyright © Astronomical Society of Pacific 2005