The milky way and the tully–fisher relation

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Abstract

We present an updated estimate of the surface density and surface brightness in B, V, I of the local Galactic disc, based on a model for the “Solar cylin-der” calibrated to reproduce Hipparcos and Tycho star counts. We discuss the mass-to-light ratio of the local stellar disc and infer the global luminosity of the Milky Way, which indicates it is underluminous with respect to the Tully–Fisher relation.

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Portinari, L., Holmberg, J., & Flynn, C. (2007). The milky way and the tully–fisher relation. In Astrophysics and Space Science Proceedings (Vol. 0, pp. 57–60). Springer Science and Business Media B.V. https://doi.org/10.1007/978-1-4020-5573-7_8

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