Exploring the evolution of giant molecular clouds in one of the nearest spiral galaxies M33
Exploring the evolution of giant molecular clouds in one of the nearest spiral galaxies M33
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Cambridge, UK: Cambridge University Press
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Language
English
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Cambridge, UK: Cambridge University Press
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The evolution of giant molecular clouds (GMCs), which are the main sites of star formation, is essential for unraveling how stars form and how galaxies evolve. We analyzed the M33 CO(J = 2–1) data with spatial resolution of 39 pc obtained by ALMA-ACA 7 m array combined with IRAM 30 m. We identified 736 GMCs and classified them into three types; Typ...
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Exploring the evolution of giant molecular clouds in one of the nearest spiral galaxies M33
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TN_cdi_proquest_journals_2823891585
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2823891585
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ISSN
1743-9213
E-ISSN
1743-9221
DOI
10.1017/S1743921322004380