The RMS Survey: 13CO observations of candidate massive YSOs in the southern hemisphere
J. S. Urquhart, A. L. Busfield, M. G. Hoare, S. L. Lumsden, R. D., Oudmaijer, T. J. T. Moore, A. G. Gibb, C. R. Purcell, M. G. Burton, L. J., L. Marechal

TL;DR
This study presents 13CO observations of 854 candidate massive young stellar objects from the RMS survey, successfully detecting emission in 88%, and deriving kinematic velocities for most sources to aid in understanding their properties.
Contribution
It provides a large dataset of 13CO observations for MYSO candidates and develops a method to resolve multiple emission components for accurate velocity assignment.
Findings
Detected 13CO emission towards 88% of sources
Unambiguously determined velocities for 80% of sources
Identified multiple emission components in 60% of sources
Abstract
Abridged: The Red MSX Source (RMS) survey is an ongoing multi-wavelength observational programme designed to return a large, well-selected sample of massive young stellar objects (MYSOs). Here we present 13CO observations made towards 854 MYSOs candidates located in the 3rd and 4th quadrants. We detected 13CO emission towards a total of 751 of the 854 RMS sources observed (~88%). In total 2185 emission components are detected above 3 level. Multiple emission profiles are observed towards the majority of these sources - 455 sources (~60%) - with an average of ~4 molecular clouds along the line of sight. These multiple emission features make it difficult to assign a kinematic velocity to many of our sample. We have used archival CS (J=2-1) and maser velocities to resolved the component multiplicity towards 82 sources and have derived a criterion which is used to identify the most…
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