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Paper: Supernova Remnants in Optical Recombination Lines
Volume: 510, Stars: From Collapse to Collapse
Page: 54
Authors: Vasiliev, E. O.; Shchekinov,Yu. A.
Abstract: Observational data of star-forming complexes are commonly represented in the 'Hα line surface brightness – velocity dispersion' diagram (I(Hα)–σ). Based on a set of 3D numerical simulations of clustered supernova remnants we discuss possible interpretations of different parts of the diagram.
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