Paper:	Dust and Chromospheres in M warfs
Volume:	448, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Page:	131
Authors:	Bessell, M. S.
Abstract:	Whilst impressive work has gone into modelling the spectra of M dwarfs over the past 10 years, there remain significant differences between the best model spectra and observations that indicate serious shortcomings in our understanding of M dwarf atmospheres. This contribution outlines the major observational differences and discusses the likelihood of dust opacity in the coolest M dwarfs and chromospheres in all M dwarfs as being explanations for the outstanding differences.

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