2001MNRAS.323L...7P


Query : 2001MNRAS.323L...7P

2001MNRAS.323L...7P - Mon. Not. R. Astron. Soc., 323, L7-L11 (2001/May-1)

Collisional excitation of H2 by grains in C-type shocks.

PINEAU DES FORETS G., FLOWER D.R., AGUILLON F., SIDIS V. and SIZUN M.

Abstract (from CDS):

We have performed classical trajectory Monte Carlo calculations of the probabilities of rovibrational excitation and dissociation of molecular hydrogen in collisions with a surface, modelled as MgO. The results show that, in C-type shock waves, states of high excitation energy are populated predominantly in collisions with charged grains, rather than with much more abundant neutral species. The intensities of rovibrational transitions of H2 have been calculated for a series of models of C-type shocks, considered to be relevant to molecular outflow sources. We compare the column densities of excited states of H2 and the intensities of representative rovibrational transitions, calculated excluding and including collisions with grains.

Abstract Copyright: The Royal Astronomical Society

Journal keyword(s): molecular data - molecular processes - shock waves - stars: formation - ISM: jets and outflows.

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 NAME OMC-1 MoC 05 35 14 -05 22.4           ~ 1249 2

Query : 2001MNRAS.323L...7P

Basic data :
NAME OMC-1 -- Molecular Cloud
Other object types:
otypes_help
MoC (OMC), DNe ([DB2002b])
ICRS coord. (ep=J2000) :
05 35 14.0 -05 22 24 [ ] E ~
FK4 coord. (ep=B1950 eq=1950) :
05 32 46.5 -05 24 17 [ ]
Gal coord. (ep=J2000) :
208.9904 -19.3858 [ ]
Angular size (arcmin):
7 4 90 (~) D 2002A&A...383..631D
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Identifiers (3) :
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NAME OMC-1 OMC 1 [DB2002b] G208.99-19.38

References (1249 between 1850 and 2026) (Total 1249)
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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