1999ApJ...518..814M


Query : 1999ApJ...518..814M

1999ApJ...518..814M - Astrophys. J., 518, 814-820 (1999/June-3)

What can the kinematic complexity of astrophysical shear flows lead to?.

MAHAJAN S.M. and ROGAVA A.D.

Abstract (from CDS):

We develop a method for investigating waves and instabilities in astrophysical shear flows with complex kinematics. Using new tools, we find an unexpected richness in the spectrum of compressible fluctuations sustained by such a flow. The principal characteristic of the revealed exotic phenomena is their asymptotic persistence in the absence of viscosity. ``Echoing'' as well as strongly unstable (including parametrically driven) solutions are identified. Examples of astrophysical shear flows with nontrivial velocity structure where these method and results can be applied are also discussed.

Abstract Copyright: ∼

Journal keyword(s): Hydrodynamics - Instabilities - Waves

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* V1213 Tau Or* 04 31 37.5055489536 +18 12 24.383952396           K7 605 0
2 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
3 V* R Aqr Sy* 23 43 49.4634303216 -15 17 04.176349872   8.823 7.683 9.37   M6.5-8.5e 823 0

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