Abstract
ABSTRACT The late-time supernova atmosphere problem is discussed in the context of standard methods and techniques used for the study of emission nebulae. Physical processes and related numerical problems peculiar to supernovae at late-times are emphasized. A brief overview of numerical methods for determining the physical state and the emergent spectrum from models of supernovae is given.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Publications of the Astronomical Society of the Pacific
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
