{ "id": "1007.1854", "version": "v1", "published": "2010-07-12T09:56:53.000Z", "updated": "2010-07-12T09:56:53.000Z", "title": "Ammonia and CO observations toward low-luminosity 6.7-GHz methanol masers", "authors": [ "Y. W. Wu", "Y. Xu", "J. D. Pandian", "J. Yang", "C. Henkel", "K. M. Menten", "S. B. Zhang" ], "comment": "37 pages, 7 figures, 9 tables accepted by ApJ", "categories": [ "astro-ph.GA" ], "abstract": "To investigate whether distinctions exist between low and high-luminosity Class II 6.7-GHz methanol masers, we have undertaken multi-line mapping observations of various molecular lines, including the NH3(1,1), (2,2), (3,3), (4,4) and 12CO(1-0) transitions, towards a sample of 9 low-luminosity 6.7-GHz masers, and 12CO (1-0) observations towards a sample of 8 high-luminosity 6.7-GHz masers, for which we already had NH3 spectral line data. Emission in the NH3 (1,1), (2,2) and (3,3) transitions was detected in 8 out of 9 low-luminosity maser sources, in which 14 cores were identified. We derive densities, column densities, temperatures, core sizes and masses of both low and high-luminosity maser regions. Comparative analysis of the physical quantities reveals marked distinctions between the low-luminosity and high-luminosity groups: in general, cores associated with high-luminosity 6.7-GHz masers are larger and more massive than those traced by low-luminosity 6.7-GHz masers; regions traced by the high-luminosity masers have larger column densities but lower densities than those of the low-luminosity maser regions. Further, strong correlations between 6.7-GHz maser luminosity and NH3(1,1) and (2,2) line widths are found, indicating that internal motions in high-luminosity maser regions are more energetic than those in low-luminosity maser regions. A 12CO (1-0) outflow analysis also shows distinctions in that outflows associated with high-luminosity masers have wider line wings and larger sizes than those associated with low-luminosity masers.", "revisions": [ { "version": "v1", "updated": "2010-07-12T09:56:53.000Z" } ], "analyses": { "keywords": [ "methanol masers", "low-luminosity maser regions", "high-luminosity maser regions", "nh3 spectral line data", "low-luminosity maser sources" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/720/1/392" }, "note": { "typesetting": "TeX", "pages": 37, "language": "en", "license": "arXiv", "status": "editable", "inspire": 860873, "adsabs": "2010arXiv1007.1854W" } } }