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The 6-GHz multibeam maser survey III: comparison between the MMB and HOPS

Breen, SL, Contreras, Y, Ellingsen, SP, Green, JA, Walsh, AJ, Avison, A, Longmore, SN, Fuller, GA, Voronkov, MA, Horton, J and Kroon, A (2017) The 6-GHz multibeam maser survey III: comparison between the MMB and HOPS. Monthly Notices of the Royal Astronomical Society, 474 (3). pp. 3898-3911. ISSN 0035-8711

1711.07589v1.pdf - Accepted Version

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We have compared the occurrence of 6.7-GHz and 12.2-GHz methanol masers with 22-GHz water masers and 6035-MHz excited-state OH masers in the 100 square degree region of the southern Galactic plane common to the Methanol Multibeam (MMB) and H2O southern Galactic Plane surveys (HOPS). We find the most populous star formation species to be 6.7-GHz methanol, followed by water, then 12.2-GHz and, finally, excited-state OH masers. We present association statistics, flux density (and luminosity where appropriate) and velocity range distributions across the largest, fully surveyed portion of the Galactic plane for four of the most common types of masers found in the vicinity of star formation regions. Comparison of the occurrence of the four maser types with far-infrared dust temperatures shows that sources exhibiting excited-state OH maser emission are warmer than sources showing any of the other three maser types. We further find that sources exhibiting both 6.7-GHz and 12.2-GHz methanol masers are warmer than sources exhibiting just 6.7-GHz methanol maser emission. These findings are consistent with previously made suggestions that both OH and 12.2-GHz methanol masers generally trace a later stage of star formation compared to other common maser types.

Item Type: Article
Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society Published by Oxford University Press on behalf of the Royal Astronomical Society.
Uncontrolled Keywords: astro-ph.GA; astro-ph.GA
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: Oxford University Press
Related URLs:
Date Deposited: 24 Nov 2017 10:44
Last Modified: 04 Sep 2021 10:57
DOI or ID number: 10.1093/mnras/stx3051
URI: https://researchonline.ljmu.ac.uk/id/eprint/7598
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