![]() ![]() We discuss the impact of our findings on the origins, circumstellar media, and observed properties of SNe Ia and magnetized white dwarfs. After the dynamical phase of the merger, magnetic stresses rapidly redistribute angular momentum, leading to nearly solid-body rotation on a viscous timescale of 10 G. (e.g., total integrated stellar mass loss) right down to the white dwarf cooling. ![]() ![]() In this paper, we present a model for the long-term evolution of the merger of two unequal mass C/O white dwarfs (WDs). Aside from the specific issue of a stellar stream corresponding to the. ![]()
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |