Stellar Astrophysics Halo stars

	Accretion Processes onto Globular Cluster Stars. Postscript
	Accretion from AGB winds Postscript
	What Happens to the Gas in Globular Clusters ? Postscript
	The Metallicity Gradient of the Old Halo Postscript
	On the Pssibility of Self-Enrichment in Globular Clusters Postscript
	Abundance Correlations in Thick Disk and Halo Stars Postscript
	Puzzling Locations of Mildly Metal-Poor Stars in the HR Diagram Postscript
	Orbital Parameters of 80 Nearby Mildly Metal-Poor Stars: a search for correlations between abundance ratios and kinematics. Postscript
	The EASE Scenario: Dynamical Study of the Supernova Phase. Postscript