Back to the Abstract

	1 Introduction
	2 Interferometric observations and data reduction
	3 Analysis of the CO maps
	4 Kinematical post-AGB lifetimes and dynamical parameters
	5 Comparison between the molecular maps and optical imaging
	6 Dependence on the distance and possible scenarios to explain Frosty Leo peculiarities
	7 Conclusions
	References
	Online Material

	List of tables
	List of figures