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- W4294934831 abstract "The J =1–0 lines of HCN and HCO + have become the default tracers of dense molecular gas in external galaxies. To study the relation between HCN and HCO + emission and density, we have mapped their J =3–2 lines with the ALMA Compact Array (ACA) in the nearby star-forming galaxies NGC3351, NGC3627, and NGC4321. Combined with archival line maps of HCN(1–0), HCO + (1–0), CO(1–0), and CO(2–1), we use this data set to: (1) compare the excitation of dense gas tracers in normal and starburst/AGN galaxies; (2) explore how line ratios vary across galaxy disks; (3) infer the density distribution and other cloud properties on a pixel-by-pixel basis through a physically-motivated radiative transfer model." @default.
- W4294934831 created "2022-09-08" @default.
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- W4294934831 date "2022-01-01" @default.
- W4294934831 modified "2023-10-14" @default.
- W4294934831 title "Multi-line modelling in nearby galaxies: The link between dense gas and star formation in different environments" @default.
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- W4294934831 doi "https://doi.org/10.1051/epjconf/202226500008" @default.
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