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  5. ATLASGAL - physical parameters of dust clumps associated with 6.7 GHz methanol masers
 

ATLASGAL - physical parameters of dust clumps associated with 6.7 GHz methanol masers

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2019
Author(s)
Billington, S. J.
•
Urquhart, J. S.
•
König, C.
•
Moore, T. J. T.
•
Eden, D. J.
•
Breen, S. L.
•
Kim, W. -J.
•
Thompson, M. A.
•
Ellingsen, S. P.
•
Menten, K. M.
•
Wyrowski, F.
•
Leurini, Silvia  
DOI
10.1093/mnras/stz2691
Abstract
We have constructed the largest sample of dust-associated class II 6.7 GHz methanol masers yet obtained. New measurements from the Methanol Multibeam (MMB) survey were combined with the 870 μ m APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) and the 850 μ m JCMT Plane Survey (JPS). Together with two previous studies we have now identified the host clumps for 958 methanol masers across the Galactic Plane, covering approximately 99 per cent of the MMB catalogue and increasing the known sample of dust-associated masers by over 30 per cent. We investigate correlations between the physical properties of the clumps and masers using distances and luminosities drawn from the literature. Clumps hosting methanol masers are significantly more compact and have higher volume densities than the general population of clumps. We determine a minimum volume density threshold of n(H2) ≥ 104 cm-3 for the efficient formation of intermediate- and high-mass stars. We find 6.7 GHz methanol masers are associated with a distinct part of the evolutionary process (Lbol/Mfwhm ratios of between 100.6 and 102.2) and have well-defined turning on and termination points. We estimate the lower limit for the mass of embedded objects to be ≥6 M☉ and the statistical lifetime of the methanol maser stage to be ∼3.3 × 104 yr. This suggests that methanol masers are indeed reliable tracers of high-mass star formation, and indicates that the evolutionary period traced by this marker is relatively rapid.
Volume
490
Issue
2
Start page
2779
Uri
http://hdl.handle.net/20.500.12386/28922
Url
https://academic.oup.com/mnras/article/490/2/2779/5583008
Issn Identifier
0035-8711
Ads BibCode
2019MNRAS.490.2779B
Rights
open.access
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