Abstract
We present observations of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes spanning to , with a latitudinal coverage of at least 210 deg, totalling an area of $. These data have been taken at 0.6 arcmin spatial resolution and 0.1 km s spectral resolution, providing an unprecedented view of the molecular gas clouds of the Southern Galactic Plane in the 109-115 GHz transitions of CO, CO, C O, and C O.
Original language | English |
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Article number | e047 |
Number of pages | 13 |
Journal | Publications of the Astronomical Society of Australia |
Volume | 40 |
DOIs | |
Publication status | Published - 22 Aug 2023 |
Bibliographical note
Publisher Copyright:© The Author(s), 2023. Published by Cambridge University Press on behalf of the Astronomical Society of Australia.
Open Access - Access Right Statement
© The Author(s), 2023. Published by Cambridge University Press on behalf of the Astronomical Society of Australia. This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.Keywords
- Galaxy: structure
- radio lines: ISM
- Galaxy: kinematics and dynamics
- ISM: molecules
- surveys
- ISM: clouds