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- W94060669 abstract "The mass and distribution of baryons in galaxies is closely related to the inferred structure of the dark halo. A robust estimate of the baryon content requires knowledge of the typical mass–to–light (M/L) ratio of the stellar component. Various arguments favour a low M * /L I < 1 for late–type spirals. We show that “bottom-light” Initial Mass Functions (IMFs) favoured by recent literature do yield so low M/L ratios, for Sbc/Sc discs. We also predict the stellar M/L ratio, and hence the zero–point of the Tully–Fisher relation, to vary significantly with Hubble disc type. Finally, we provide colour–M/L relations to derive the stellar M/L ratio from the observed photometry, for different IMFs." @default.
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- W94060669 date "2004-01-01" @default.
- W94060669 modified "2023-10-11" @default.
- W94060669 title "The stellar Mass–to–Light ratio in disc galaxies" @default.
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- W94060669 doi "https://doi.org/10.1017/s0074180900183457" @default.
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