Rotational Instabilities and Stellar Evolution
نویسندگان
چکیده
منابع مشابه
Rotational Instabilities in Post–Collapse Stellar Cores
A core–collapse supernova might produce large amplitude gravitational waves if, through the collapse process, the inner core can aquire enough rotational energy to become dynamically unstable. In this report I present the results of 3-D numerical simulations of core collapse supernovae. These simulations indicate that for some initial conditions the post–collapse inner core is indeed unstable. ...
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R. P. Drake, C. C. Kuranz, A. R. Miles, H. J. Muthsam, and T. Plewa University of Michigan, 2455 Hayward St., Ann Arbor, Michigan 48109, USA Lawrence Livermore National Laboratory, 7500 East Ave., Livermore, California 94550, USA Faculty of Mathematics, University of Vienna, Nordbergstr. 15, A-1090 Vienna, Austria School of Computational Science, Florida State University, DSL 443, Tallahassee, ...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1974
ISSN: 0074-1809
DOI: 10.1017/s0074180900237492