INVESTIGATION OF DENSE GAS TOWARDS RELATIVISTIC OUTFLOW SOURCES

Author:

HAWKES J.1,ROWELL G.1,DAWSON B.1,AHARONIAN F.2,BURTON M.3,FUKUI Y.4,FURUKAWA N.4,HAYAKAWA T.4,KAWAMURA A.4,MAXTED N.1,de OÑA-WILHELMI E.2,de WILT P.1,WALSH A.5

Affiliation:

1. School of Chemistry and Physics, University of Adelaide, SA, 5005, Australia

2. Max-Planck Institut für Kernphysik, P.O. Box 103980, D-69029 Heidelberg, Germany

3. School of Physics, University of New South Wales, Sydney 2052, Australia

4. Dept. Astrophysics, Nagoya University, Chikusa-ku, Nagoya, 464-8062, Japan

5. International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth, Australia

Abstract

We probe the interstellar medium towards the objects Circinus X-1, a low-mass X-ray binary with relativistic jets; and the highly energetic Westerlund 2 stellar cluster, which is located towards TeV gamma-ray emission and interesting arc- and jet-like features seen in Nanten 12CO data. We have mapped both regions with the Mopra radio telescope, in 7 mm and 12 mm wavebands, looking for evidence of disrupted/dense gas caused by the interaction between high energy outflows and the ISM. Towards Westerlund 2, peaks in CS(J=1-0) emission indicate high density gas towards the middle of the arc and the endpoint of the jet; and radio recombination line emission is seen overlapping the coincident HII region RCW49. Towards Circinus X-1, 12CO(J = 1-0) Nanten data reveals three molecular clouds that lie in the region of Cir X-1. Gas parameters for each cloud are presented here.

Publisher

World Scientific Pub Co Pte Lt

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