2005MNRAS.358.1195S

Query : 2005MNRAS.358.1195S

2005MNRAS.358.1195S - Mon. Not. R. Astron. Soc., 358, 1195-1214 (2005/April-3)

A simple model for H2line profiles in bow shocks.

SCHULTZ A.S.B., BURTON M.G. and BRAND P.W.J.L.

Abstract (from CDS):

We present a model for empirically reproducing line profiles of molecular hydrogen emission in bow shocks. The model takes into account bow velocity, dissociation limit, a cooling function, viewing angle, bow shape and a limited form of extinction. Our results show that both geometrical factors and shock physics can significantly affect the profile morphology. In a companion paper we will apply this model to Fabry-Perot observations of bow shocks in the Orion BN-KL outflow.

Abstract Copyright: 2005 RAS

Journal keyword(s): line: profiles - shock waves - stars: formation - ISM: jets and outflows - ISM: molecules

Simbad objects: 5

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Number of rows : 5
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 2MASS J03290842+3115284 NIR 03 29 08.420 +31 15 28.48           ~ 229 1
2 NAME Orion-KL SFR 05 35 14.16 -05 22 21.5           ~ 2421 1
3 HH 34 HH 05 35 31.30 -06 28 43.0     16     ~ 493 2
4 HH 1 HH 05 36 20.8 -06 45 13           ~ 415 1
5 HH 47 HH 08 25 44.30 -51 00 26.2           ~ 247 0

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