2002MNRAS.333....1W

Query : 2002MNRAS.333....1W

2002MNRAS.333....1W - Mon. Not. R. Astron. Soc., 333, 1-8 (2002/June-2)

Resolved shocks in clumpy media.

WILLIAMS R.J.R. and DYSON J.E.

Abstract (from CDS):

We study the structure of shocks in clumpy media, using a multifluid formalism. As expected, shocks broaden as they weaken: for sufficiently weak shocks, no viscous subshock appears in the structure. This has significant implications for the survival of dense clouds in regions overrun by shocks in a wide range of astrophysical circumstances, from planetary nebulae to the nuclei of starburst galaxies.

Abstract Copyright: 2002 Blackwell Science Ltd

Journal keyword(s): hydrodynamics - shock waves - ISM: clouds - ISM: globules - ISM: kinematics and dynamics

Simbad objects: 4

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Number of rows : 4
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 M 42 HII 05 35 16.8 -05 23 15           ~ 4411 0
2 NAME Ori A MoC 05 38 -07.1           ~ 3187 0
3 PN A66 30 PN 08 46 53.4639874872 +17 52 46.369394580   14.23 14.30 13.47   [WC5] 431 0
4 * eta Car s*b 10 45 03.545808 -59 41 03.95124 6.37 7.03 6.48 6.123 4.41 LBV 2543 0

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