K. Cubuk, M. Burton, C. Braiding, G. Wong, G. Rowell, N. Maxted, D. Eden, R. Z. E. Alsaberi, R. Blackwell, R. Enokiya, K. Feijen, M. Filipović, M. Freeman, S. Fujita, M. Ghavam, B. Gunay, B. Indermuehle, K. Hayashi, M. Kohno, T. Nagaya, A. Nishimura, K. Okawa, D. Rebolledo, D. Romano, H. Sano, C. Snoswell, N. Tothill, K. Tsuge, F. Voisin, Y. Yamane, S. Yoshiike
{"title":"The Mopra Southern Galactic Plane CO Survey – data release 4– complete survey","authors":"K. Cubuk, M. Burton, C. Braiding, G. Wong, G. Rowell, N. Maxted, D. Eden, R. Z. E. Alsaberi, R. Blackwell, R. Enokiya, K. Feijen, M. Filipović, M. Freeman, S. Fujita, M. Ghavam, B. Gunay, B. Indermuehle, K. Hayashi, M. Kohno, T. Nagaya, A. Nishimura, K. Okawa, D. Rebolledo, D. Romano, H. Sano, C. Snoswell, N. Tothill, K. Tsuge, F. Voisin, Y. Yamane, S. Yoshiike","doi":"10.1017/pasa.2023.44","DOIUrl":null,"url":null,"abstract":"Abstract We present observations of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes spanning \n$l = 250^{\\circ}$\n ( \n$-110^{\\circ}$\n ) to \n$l = 355^{\\circ}$\n ( \n$-5^{\\circ}$\n ), with a latitudinal coverage of at least \n$|b|<1^\\circ$\n , totalling an area of \n$>$\n 210 deg \n$^{2}$\n . These data have been taken at 0.6 arcmin spatial resolution and 0.1 km s \n$^{-1}$\n spectral resolution, providing an unprecedented view of the molecular gas clouds of the Southern Galactic Plane in the 109–115 GHz \n$J = 1-0$\n transitions of \n$^{12}$\n CO, \n$^{13}$\n CO, C \n$^{18}$\n O, and C \n$^{17}$\n O.","PeriodicalId":20753,"journal":{"name":"Publications of the Astronomical Society of Australia","volume":null,"pages":null},"PeriodicalIF":4.5000,"publicationDate":"2023-08-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Publications of the Astronomical Society of Australia","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1017/pasa.2023.44","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Abstract We present observations of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes spanning
$l = 250^{\circ}$
(
$-110^{\circ}$
) to
$l = 355^{\circ}$
(
$-5^{\circ}$
), with a latitudinal coverage of at least
$|b|<1^\circ$
, totalling an area of
$>$
210 deg
$^{2}$
. These data have been taken at 0.6 arcmin spatial resolution and 0.1 km s
$^{-1}$
spectral resolution, providing an unprecedented view of the molecular gas clouds of the Southern Galactic Plane in the 109–115 GHz
$J = 1-0$
transitions of
$^{12}$
CO,
$^{13}$
CO, C
$^{18}$
O, and C
$^{17}$
O.
期刊介绍：
Publications of the Astronomical Society of Australia (PASA) publishes new and significant research in astronomy and astrophysics. PASA covers a wide range of topics within astronomy, including multi-wavelength observations, theoretical modelling, computational astronomy and visualisation. PASA also maintains its heritage of publishing results on southern hemisphere astronomy and on astronomy with Australian facilities.
PASA publishes research papers, review papers and special series on topical issues, making use of expert international reviewers and an experienced Editorial Board. As an electronic-only journal, PASA publishes paper by paper, ensuring a rapid publication rate. There are no page charges. PASA''s Editorial Board approve a certain number of papers per year to be published Open Access without a publication fee.
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