Time	Speaker	Title
Chairman	Francesco Palla	Resolving Local Galaxies: SFR tracers and the gas-SFR relation
8:45-9:15	Kennicutt Robert	Lesson from the First 50 Years
9:15-9:40	Calzetti Daniela	SFR estimates across the electromagnetic spectrum
9:40-9:55	Dumas Gaelle	Star formation rates on 100pc scale in M51: a multi-wavelength point of view
9:55-10:20	Bigiel Frank	The SF law on sub-kpc scales - from the inner disks to the outskirts of nearby galaxies
10:20-10:45	Leroy Adam	Results From HERACLES and THINGS: Where is the ISM good at forming stars?
10.45 - 11.15		Coffee Break in Voliera
11:15-11:40	Gao Yu	The Star Formation Law in Dense Gas: the Far-IR and HCN Correlation
11:40-11:55	Narayanan Desika	Molecular Star Formation Rate Laws in Galaxies
11:55-12:10	Santangelo Gina	Resolving the molecular environment of super star clusters in Henize2-10
12:10-12:25	Juneau Stephanie	Enhanced Dense Gas Fraction in Luminous Infrared Galaxies
12:25-12:40	Wilson Christine	Tracing the fuel for star formation: results from the ngls
12:40-12:55	Vlahakis Catherine	Investigating the spatially resolved star formation process using a HARP-B CO(3-2) map of M51.
13:00-14:00		Lunch
Chairman	Andi Burkert	Theory on SFR: from disks to GMCs
16:30-16:55	Wada Keiichi	Relations between the Global SFR and Intrinsic Structures of the ISM in Galactic Disks
16:55-17:20	Zasov Anatoly	The Schmidt law: how universal is it?
17:20-17:45	Krumholz Mark	Physical Origins of the Star Formation Law
17:45-18:10	Ostriker Eve	Regulation of star formation in disk galaxies: dynamical effects
18:10-18:40		Coffee Break in Cortile
18:40-19:05	Tasker Elizabeth	Star Formation and the evolution of GMCs in global disk galaxy simulations
19:05-19:30	Tan Jonathan	Star formation rates in disk galaxies and circumnuclear starbursts from cloud collisions
19:30-19:45	Dobbs Clare	A simple model for the relationship between star formation and surface density
20:00-22:00		Cena nella Sala Capitolare dell'Abbazia