2002ApJ...576..814G


Query : 2002ApJ...576..814G

2002ApJ...576..814G - Astrophys. J., 576, 814-831 (2002/September-2)

Tentative detection of molecular oxygen in the ρ Ophiuchi cloud.

GOLDSMITH P.F., LI D., BERGIN E.A., MELNICK G.J., TOLLS V., HOWE J.E., SNELL R.L. and NEUFELD D.A.

Abstract (from CDS):

We report the tentative detection of molecular oxygen in the interstellar medium. Deep integrations using the Submillimeter Wave Astronomy (SWAS) satellite of the ρ Oph A cloud have resulted in a detection of an emission feature consistent with the NJ=33⟶12transition of O2 at a local standard of rest velocity of 6.0 km.s–1. The line width and velocity are suggestive of the redshifted wing emission seen in species that trace the molecular outflows seen in this region. The fractional abundance of O2relative to H2in this high-velocity gas is approximately 10–5. The fractional abundance of ortho-H2O in this material is 8x10–8, somewhat higher than found in quiescent material by earlier SWAS observations but less than that found in younger outflows. We suggest a unified scenario that explains the low O2abundance in cloud cores previously reported [X(O2)≤fewx10–7], along with the much enhanced abundance in the outflow region. In this picture, quiescent clouds are characterized by significant depletion of gas-phase oxygen, which ends up largely as water ice on the dust grains. A shock associated with the outflow results in almost all oxygen being processed into gas-phase water. In the cool postshock gas, the standard gas-phase chemistry reasserts itself, and after an elapsed time of a few times 105 yr, the O2abundance has increased to the point that this species is one of the main repositories of oxygen atoms. At the same time, the gas-phase water abundance drops drastically, in agreement with the SWAS observations that we report here. On a somewhat longer timescale, depletion again dominates and the gas-phase abundance of O2drops by several orders of magnitude, with a significant fraction of oxygen remaining in atomic form.

Abstract Copyright:

Journal keyword(s): Astrochemistry - ISM: Clouds - ISM: Individual: Name: ρ Ophiuchi Cloud - ISM: Molecules - Molecular Processes - Submillimeter

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 NAME Orion-KL SFR 05 35 14.16 -05 22 21.5           ~ 2165 1
2 NAME Orion Molecular Cloud MoC 05 56 -01.8           ~ 1000 1
3 GSS 30 Y*O 16 26 21.38160 -24 23 04.0524           ~ 207 1
4 NAME rho Oph A Cloud MoC 16 26 26.4 -24 22 33           ~ 280 1
5 GSS 35 TT* 16 26 34.1761719864 -24 23 28.283473860     16.53 14.75 12.51 B3 230 1
6 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3373 1

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2022.08.10-07:30:34

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