1.
Astrophys J
; 527(2): L113-L116, 1999 Dec 20.
Artículo
en Inglés
| MEDLINE
| ID: mdl-10577952
RESUMEN
We present results from the first three-dimensional numerical simulations of moderately supersonic cloud motion through a tenuous, magnetized medium. We show that the interaction of the cloud with a magnetic field perpendicular to its motion has a great dynamical impact on the development of instabilities at the cloud surface. Even for initially spherical clouds, magnetic field lines become trapped in surface deformations and undergo stretching. The consequent field amplification that occurs there and, in particular, its variation across the cloud face then dramatically enhance the growth rate of Rayleigh-Taylor unstable modes, hastening the cloud disruption.
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3.
Phys Rev D Part Fields
; 43(4): 1413-1415, 1991 Feb 15.
Artículo
en Inglés
| MEDLINE
| ID: mdl-10013512
4.
Phys Rev D Part Fields
; 42(9): 2974-2976, 1990 Nov 01.
Artículo
en Inglés
| MEDLINE
| ID: mdl-10013179
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7.
Phys Rev D Part Fields
; 38(3): 768-775, 1988 Aug 01.
Artículo
en Inglés
| MEDLINE
| ID: mdl-9959205
8.
Phys Rev D Part Fields
; 37(12): 3361-3363, 1988 Jun 15.
Artículo
en Inglés
| MEDLINE
| ID: mdl-9958631
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10.
Phys Rev D Part Fields
; 35(7): 2073-2076, 1987 Apr 01.
Artículo
en Inglés
| MEDLINE
| ID: mdl-9957895
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