Rayleigh-Taylor instability in the asymmetric supernova explosion

Shoichi Yamada, Katsuhiko Sato

Research output: Contribution to journalArticle

19 Citations (Scopus)

Abstract

We studied matter mixing by Rayleigh-Taylor instability in the jetlike supernova explosion by numerical calculations of two-dimensional hydrodynamics. We found that (1) the asymmetric explosion with 5% initial perturbation causes the same degree of matter mixing as the spherical one with 30% perturbation, and that (2) 30% initial perturbation in the jetlike explosion is sufficient to explain the mixing in SN 1987A suggested by many observations without any subsequent instability such as nickel bubble formation.

Original languageEnglish
Pages (from-to)594-602
Number of pages9
JournalAstrophysical Journal
Volume382
Issue number2
Publication statusPublished - 1991 Dec 1
Externally publishedYes

Fingerprint

Taylor instability
supernovae
explosions
explosion
perturbation
bubble
nickel
bubbles
hydrodynamics
causes

Keywords

  • Hydrodynamics
  • Stars: individual (SN 1987A)
  • Stars: interiors
  • Stars: supernovae

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Rayleigh-Taylor instability in the asymmetric supernova explosion. / Yamada, Shoichi; Sato, Katsuhiko.

In: Astrophysical Journal, Vol. 382, No. 2, 01.12.1991, p. 594-602.

Research output: Contribution to journalArticle

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