A&A 430, 549-560 (2005)
DOI: 10.1051/0004-6361:20040437
The interstellar C
O/C
O ratio in the solar
neighbourhood:
The
Ophiuchus cloud
J. G. A. Wouterloot1, 2, J. Brand3 and C. Henkel4
1 Joint Astronomy Centre, 660 N. A'ohoku Place, University Park, 96720 Hilo, Hawaii, USA
e-mail: j.wouterloot@jach.hawaii.edu
2 Radioastronomisches Institut, Univ. Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
3 Istituto di Radioastronomia, CNR, via Gobetti 101, 40129 Bologna, Italy
4 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
(Received 13 March 2004 / Accepted 15 September 2004)
Abstract
Observations of up to ten carbon monoxide (CO and isotopomers) transitions are
presented to study the interstellar C
18O/C
17O ratio towards 21 positions
in the nearby (
pc) low-mass star forming cloud
Oph.
A map of the C
18O
J=1-0 distribution of parts of the cloud is also
shown.
An average
12C
18O/
12C
17O isotopomeric ratio of
,
reflecting the
18O/
17O isotope ratio,
is derived from Large Velocity Gradient (LVG) calculations. From LTE column
densities we derive a ratio of
.
These calculations also show that the kinetic temperature decreases
from about 30 K in the cloud envelope to about 10 K in the cloud cores. This decrease is
accompanied by an increase of the average molecular hydrogen density
from 10
4 cm
-3 to
10
5 cm
-3. Towards some lines of sight
C
18O optical depths reach values of order unity.
Key words: ISM: abundances -- ISM: clouds -- ISM: molecules -- Galaxy: abundances -- radio lines: ISM -- ISM: individual objects: rho Oph
SIMBAD Objects
© ESO 2005
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