A 7 mm line survey of the shocked and disrupted molecular gas towards the W28 field TeV gamma-ray sources
Article first published online: 2 NOV 2011
© 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS
Monthly Notices of the Royal Astronomical Society
Volume 419, Issue 1, pages 251–266, January 2012
How to Cite
Nicholas, B. P., Rowell, G., Burton, M. G., Walsh, A. J., Fukui, Y., Kawamura, A. and Maxted, N. I. (2012), A 7 mm line survey of the shocked and disrupted molecular gas towards the W28 field TeV gamma-ray sources. Monthly Notices of the Royal Astronomical Society, 419: 251–266. doi: 10.1111/j.1365-2966.2011.19688.x
- Issue published online: 13 DEC 2011
- Article first published online: 2 NOV 2011
- Accepted 2011 August 24. Received 2011 August 21; in original form 2011 May 28
Figure A1. Spectra for the line emission detected towards the IRAS 17589-2312 star formation core from mapping data.
Figure A2. Spectra of the SiO(1--0) v = 1, 2, 3 lines coming from the V5357Sgr Variable Star of Mira Cet type.
Figure A3. Image showing the relationship between the diffuse and dense gas in the NE cloud.
Table A1. Line parameters from a Gaussian fit to the spectra, for lines detected in deep pointing observations.
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