| Abstract | PDF (465.6 KB) | PS (5.497 MB) | References | HTML | Simbad Objects | NASA ADS Abstract Service |
A&A 482, 849-853 (2008)
DOI: 10.1051/0004-6361:200809436
Odin observations of the Galactic centre in the 118-GHz band
Upper limit to the O2 abundance
Aa. Sandqvist1, B. Larsson1, Å. Hjalmarson2, P. Bergman2, P. Bernath3, U. Frisk4, M. Olberg2, L. Pagani5, and L. M. Ziurys61 Stockholm Observatory, AlbaNova University Center, 106 91 Stockholm, Sweden
e-mail: aage@astro.su.se
2 Onsala Space Observatory, 439 92 Onsala, Sweden
3 Department of Chemistry, University of York, Heslington, York YO10 5DD, UK
4 Swedish Space Corporation, PO Box 4207, 171 04 Solna, Sweden
5 LERMA & UMR8112 du CNRS, Observatoire de Paris, 61 Av. de l'Observatoire, 75014 Paris, France
6 Arizona Radio Observatory, Steward Observatory, University of Arizona, Tucson, AZ 85721, USA
(Received 22 January 2008 / Accepted 23 February 2008)
Abstract
Aims. The Odin satellite has been used to search for the 118.75-GHz
line of molecular oxygen (O2) in the Galactic centre.
Methods. Odin observations were performed towards the Sgr
circumnuclear
disk (CND), and the Sgr A +20 km s-1 and +50 km s-1 molecular clouds
using the position-switching mode. Supplementary ground-based
observations were carried out in the 2-mm band using the ARO Kitt
Peak 12-m telescope to examine suspected SiC features.
Results. A strong emission line was found at 118.27 GHz, attributable to the
J = 13-12
HC3N line. Upper limits are presented for the 118.75-GHz O2
(11-10) ground transition line and for the 118.11-GHz
, J = 3-2 ground state SiC line at the Galactic centre. Upper limits are also presented for the 487-GHz O2 line in
the Sgr A +50 km s-1 cloud and for the 157-GHz, J = 4-3, SiC line in the
Sgr A +20 and +50 km s-1 clouds, as well as the
CND. The CH3OH line complex at 157.2-157.3 GHz has been detected in the +20 and
+50 km s-1 clouds but not towards Sgr
/CND.
Conclusions. A
upper limit for the fractional abundance ratio of [O2] /[H2] is
found to be X(O2)
1.2
10-7 towards the Sgr A molecular belt region.
Key words: Galaxy: center -- ISM: individual objects: Sgr A -- ISM: molecules -- ISM: clouds -- ISM: abundances
© ESO 2008



Document 