The Mopra Southern Galactic Plane CO Survey-data release 4-complete survey

K.O. Cubuk, M.G. Burton, C. Braiding, G. F. Wong, G. Rowell, N.I. Maxted, D. Eden, R.Z.E. Alsaberi, R. Blackwell, R. Enokiya, K. Feijen, M.D. Filipovic, M.S.R. Freeman, S. Fujita, M. Ghavam, B. Gunay, B. Indermuehle, K. Hayashi, M. Kohno, T. NagayaA. Nishimura, K. Okawa, D. Rebolledo, D. Romano, H. Sano, C. Snoswell, N.F.H. Tothill, K. Tsuge, F. Voisin, Y. Yamane, S. Yoshiike

Research output: Contribution to journalArticlepeer-review

5 Citations (Scopus)

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 languageEnglish
Article numbere047
Number of pages13
JournalPublications of the Astronomical Society of Australia
Volume40
DOIs
Publication statusPublished - 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

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