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24 April 2024
 
  » arxiv » 1501.6650

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MALT-45: A 7 mm survey of the southern Galaxy - I. Techniques and spectral line data
Christopher H. Jordan ; Andrew J. Walsh ; Vicki Lowe ; Maxim A. Voronkov ; Simon P. Ellingsen ; Shari L. Breen ; Cormac R. Purcell ; Peter J. Barnes ; Michael G. Burton ; Maria R. Cunningham ; Tracey Hill ; James M. Jackson ; Steven N. Longmore ; Nicolas Peretto ; James S.Urquhart ;
Date 27 Jan 2015
AbstractWe present the first results from the MALT-45 (Millimetre Astronomer’s Legacy Team - 45 GHz) Galactic Plane survey. We have observed 5 square-degrees ($l = 330 - 335$, $b = pm0.5$) for spectral lines in the 7 mm band (42-44 and 48-49 GHz), including $ ext{CS}$ $(1-0)$, class I $ ext{CH}_3 ext{OH}$ masers in the $7(0,7)-6(1,6)$ $ ext{A}^{+}$ transition and $ ext{SiO}$ $(1-0)$ $v=0,1,2,3$. MALT-45 is the first unbiased, large-scale, sensitive spectral line survey in this frequency range. In this paper, we present data from the survey as well as a few intriguing results; rigorous analyses of these science cases are reserved for future publications. Across the survey region, we detected 77 class I $ ext{CH}_3 ext{OH}$ masers, of which 58 are new detections, along with many sites of thermal and maser $ ext{SiO}$ emission and thermal $ ext{CS}$. We found that 35 class I $ ext{CH}_3 ext{OH}$ masers were associated with the published locations of class II $ ext{CH}_3 ext{OH}$, $ ext{H}_2 ext{O}$ and $ ext{OH}$ masers but 42 have no known masers within 60 arcsec. We compared the MALT-45 $ ext{CS}$ with $ ext{NH}_3$ (1,1) to reveal regions of $ ext{CS}$ depletion and high opacity, as well as evolved star-forming regions with a high ratio of $ ext{CS}$ to $ ext{NH}_3$. All $ ext{SiO}$ masers are new detections, and appear to be associated with evolved stars from the $it{Spitzer}$ Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE). Generally, within $ ext{SiO}$ regions of multiple vibrational modes, the intensity decreases as $v=1,2,3$, but there are a few exceptions where $v=2$ is stronger than $v=1$.
Source arXiv, 1501.6650
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