MALT-45: A 7 mm survey of the southern Galaxy - I. Techniques and spectral line data
arXiv:1501.06650 · doi:10.1093/mnras/stv178
Abstract
We present the first results from the MALT-45 (Millimetre Astronomer's Legacy Team - 45 GHz) Galactic Plane survey. We have observed 5 square-degrees (, ) for spectral lines in the 7 mm band (42-44 and 48-49 GHz), including , class I masers in the transition and . 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 masers, of which 58 are new detections, along with many sites of thermal and maser emission and thermal . We found that 35 class I masers were associated with the published locations of class II , and masers but 42 have no known masers within 60 arcsec. We compared the MALT-45 with (1,1) to reveal regions of depletion and high opacity, as well as evolved star-forming regions with a high ratio of to . All masers are new detections, and appear to be associated with evolved stars from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE). Generally, within regions of multiple vibrational modes, the intensity decreases as , but there are a few exceptions where is stronger than .
arXiv commentAccepted by Monthly Notices of the Royal Astronomical Society on 2015 January 23. Appendices will be published with MNRAS
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