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Cloud-scale elemental abundance variations and the CO-to-dust-mass conversion factor in M31 (2025)

First Author: Bosomworth C

Attributed to: Chemodynamical Simulations of the Milky Way funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stae2805

Publication URI: http://dx.doi.org/10.1093/mnras/stae2805

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4