2007AJ....134..511V


Query : 2007AJ....134..511V

2007AJ....134..511V - Astron. J., 134, 511-515 (2007/August-0)

A test of pressure equilibrium outside and inside some dust-emitting filaments and a shell.

VALLEE J.P.

Abstract (from CDS):

We have found relations characterizing two large filaments embedded in hot cavities and a shell surrounding a hot cavity. These data come from multiconstituent (gas/dust/field) homogeneous maps of the same objects modeled in the same manner. We find that the total external pressure of the cavity environment surrounding our filaments and shell is large and about equal to the total internal pressure inside the filaments and the shell. Also, we find that the filament width decreases with increasing total pressure. We expect that our work will provide a deeper insight into the origin and properties of filaments and the surrounding large-scale structure. Models of filaments neglecting a strong pressure from the outside environment would need modifications. Models requiring strong magnetism inside the filaments or shell, sufficiently strong to contain gas turbulence, do not seem to be favored by our thin filaments or shell.

Abstract Copyright: ∼

Journal keyword(s): ISM: Dust, Extinction - Infrared: ISM - ISM: Magnetic Fields - Polarization - Stars: Formation

Simbad objects: 9

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Number of rows : 9
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 NAME Barnard's Loop HII 05 27.5 -03 58           ~ 131 1
2 NAME OMC-1 MoC 05 35 14 -05 22.4           ~ 1249 2
3 OMC 3 MoC 05 35 20.0 -05 01 00           ~ 301 1
4 NAME Orion Molecular Cloud MoC 05 56 -01.8           ~ 1227 1
5 [CCE98b] 011.11-0.12 Cld 18 10.5 -19 23           ~ 119 2
6 SH 2-106 HII 20 27 26.8 +37 22 49           ~ 453 1
7 DR 21 (OH) cor 20 39 01.01 +42 22 50.2           ~ 427 0
8 DR 21 SFR 20 39 01.6 +42 19 38           O4.5 1121 0
9 LDN 1082 DNe 20 51.1 +60 11           ~ 36 0

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