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ATLASGAL – molecular fingerprints of a sample of massive star-forming clumps

Urquhart, J.S., Figura, C.C., Wyrowski, F., Giannetti, A., Kim, W.-J., Wienen, M., Leurini, S., Pillai, T., Csengeri, T., Gibson, Stuart J., and others. (2019) ATLASGAL – molecular fingerprints of a sample of massive star-forming clumps. Monthly Notices of the Royal Astronomical Society, 484 (4). pp. 4444-4470. ISSN 0035-8711. (doi:10.1093/mnras/stz154)

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Abstract

We have conducted a 3-mm molecular-line survey towards 570 high-mass star-forming clumps, using the Mopra telescope. The sample is selected from the 10,000 clumps identified by the ATLASGAL survey and includes all of the most important embedded evolutionary stages associated with massive star formation, classified into five distinct categories (quiescent, protostellar, young stellar objects, HII regions and photo-dominated regions). The observations were performed in broadband mode with frequency coverage of 85.2 to 93.4 GHz and a velocity resolution of ?0.9 km s

Item Type: Article
DOI/Identification number: 10.1093/mnras/stz154
Uncontrolled keywords: Stars: formation – Stars: early-type – ISM: clouds – ISM: submillimetre – ISM:HII regions.
Divisions: Faculties > Sciences > School of Physical Sciences
Depositing User: James Urquhart
Date Deposited: 14 Jan 2019 09:29 UTC
Last Modified: 30 May 2019 08:44 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/71636 (The current URI for this page, for reference purposes)
Urquhart, J.S.: https://orcid.org/0000-0002-1605-8050
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