Abstract
From models of plane-parallel radiating shock waves and the observations of Osterbrock and Dufour, the abundances of oxygen, nitrogen, neon and sulfur (and indirectly, or carbon) are derived for the Large Magellanic Cloud supernova remnant N49. These are somewhat smaller than solar values, and it is concluded that the discrepancies between these and values derived for the LMC H II regions reflect the composition of ''ice'' grains with low sublimation temperatures which are destroyed in the supernova event. (AIP)
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 callDisclaimer: 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.
