WISDOM Project – XXVII. Giant molecular clouds of the lenticular galaxy NGC 1387: similarities with spiral galaxy clouds

Liang, Fu-Heng, Bureau, Martin, Liu, Lijie, Dominiak, Pandora, Choi, Woorak, Davis, Timothy A. ORCID: https://orcid.org/0000-0003-4932-9379, Elford, Jacob, Gensior, Jindra, Lu, Anan, Ruffa, Ilaria, Topal, Selçuk, Williams, Thomas G and Zhang, Hengyue 2026. WISDOM Project – XXVII. Giant molecular clouds of the lenticular galaxy NGC 1387: similarities with spiral galaxy clouds. Monthly Notices of the Royal Astronomical Society , stag221. 10.1093/mnras/stag221

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Abstract

Molecular gas is crucial to understanding star formation and galaxy evolution, but the giant molecular clouds (GMCs) of early-type galaxies (ETGs) have rarely been studied. Here we present analyses of the spatially resolved GMCs of the lenticular galaxy NGC 1387, exploiting high spatial resolution (0″.15 or 14 pc) 12CO(2-1) line observations from the Atacama Large Millimeter/submillimeter Array. We identify 1285 individual GMCs and measure the fundamental properties (radius, velocity dispersion and molecular gas mass) of each with a modified version of the CPROPStoo package. Unusually for an ETG, the GMCs of NGC 1387 follow scaling relations very similar to those of the Milky Way disc and Local Group galaxy clouds, and most are virialised. GMCs with large masses and radii and/or small galactocentric distances have their angular momenta aligned with the large-scale galactic rotation, while other GMCs do not. These results show that ETGs have more diversified GMC properties than previously thought. We discuss potential reasons for such diversity, and viewing-angle dependency is a plausible candidate.

Item Type:	Article
Date Type:	Published Online
Status:	In Press
Schools:	Schools > Physics and Astronomy
Publisher:	Oxford University Press (OUP)
ISSN:	0035-8711
Date of First Compliant Deposit:	9 February 2026
Date of Acceptance:	28 January 2026
Last Modified:	11 Feb 2026 14:55
URI:	https://orca.cardiff.ac.uk/id/eprint/184543

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