2003A&A...399..553Y


Query : 2003A&A...399..553Y

2003A&A...399..553Y - Astronomy and Astrophysics, volume 399553-565 (2003/2-4)

Turbulent diffusion and mixing in interstellar dark clouds with adsorption onto grains.

YATE C.J. and MILLAR T.J.

Abstract (from CDS):

This paper reports the results of models of dark cloud chemistry incorporating a depth dependent density distribution with diffusive mixing and adsorption onto grains. The model is based on the approach taken by Xie et al. (1995ApJ...440..674X), with the addition of grain accretion effects. Without diffusion, the central regions of the cloud freeze out in less than 107 years. Freeze-out time is dependent on density, so the diffuse outer region of the cloud remains abundant in gas for about an order of magnitude longer. We find that fairly small amounts of diffusive mixing can delay freeze-out at the centre of the model cloud for a time up to an order of magnitude greater than without diffusion, due to material diffusing inward from the edges of the cloud. The gas-phase lifetime of the cloud core can thus be increased by up to an order of magnitude or more by this process. We have run three different grain models with various diffusion coefficients to investigate the effects of changing the sticking parameters.

Abstract Copyright: ∼

Journal keyword(s): astrochemistry - turbulence - diffusion - ISM: abundances - ISM: dust, extinction

Simbad objects: 1

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Number of rows : 1
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 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0

Query : 2003A&A...399..553Y

Basic data :
TMC-1 -- Molecular Cloud
Other object types:
otypes_help
PoC (MLB,[MOH94]), MoC (TMC), Cld (HCL)
ICRS coord. (ep=J2000) :
04 41 45.9 +25 41 27 [ ] D 1983ApJ...264..517M
FK4 coord. (ep=B1950 eq=1950) :
04 38 42.0 +25 35 45 [ ]
Gal coord. (ep=J2000) :
174.3852 -13.4312 [ ]
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Hierarchy : number of linked objects
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: 12
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Identifiers (4) :
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HCL 2 MLB 3-28 TMC-1 [MOH94] 6

References (1872 between 1850 and 2026) (Total 1872)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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