Back to the Abstract

	1 Introduction
	2 Observational data
	3 Analysis
	4 Mass-loss rate as a function of bolometric luminosity and stellar effective temperature
	5 The Hertzsprung-Russell diagram of dust-enshrouded AGB stars and red supergiants
	6 Summary
	Appendix A: Spectra of galactic M-type stars
	References

	List of tables
	List of figures