Abstract
We present self-similar solutions for remnants that are mass-loaded by conductively driven evaporation. This work extends the earlier results of Chieze and Lazareff through the inclusion of the explicit dependence of the mass-loading rate on position as well as temperature, and the treatment of cylindrically symmetric as well as spherically symmetric cases. The latter case is relevant to an individual supernova remnant in its adiabatic phase expanding into a clumpy interstellar medium. The former case may be relevant to the evolution of the outflow from a young galaxy in which a nearly simultaneous burst of star formation occurs as the density increases on its axis of symmetry.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
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.