Program (last updated: Oct 10)

Program in pdf

Oct 10, Monday
9:10 – 9:50 Introduction Thomas Henning
09:50 – 10:10 Planet formation in young multiple systems Stéphane Guilloteau
10:10 – 11:25 coffee break  
11:25 – 11:45 Surface Density Perturbations in TW Hya Traced by Molecular Emission Richard Teague
11:45 – 12:05 Small disks observed with ALMA Stéphane Guilloteau
12:05 – 12:25 Mid-infrared variability of young stellar objects: implications for inner disk structure Péter Ábrahám
12:25 – 14:25 lunch break (optional program at 13:50: 3D video presentation)  
14:25 - 15:00 The Long Way From Dust to Planetesimals Til Birnstiel
15:00 – 15:20 Chemistry of cold dense cores and initial conditions for disks chemistry Maxime Ruaud
15:20 – 15:40 The role of surface chemistry and non-LTE in methanol line excitation in TW Hya Dmitry Semenov
15:40 – 16:40 coffee break  
16:40 – 17:15 Lifetime of the solar nebula constrained by meteorite paleomagnetism Benjamin P. Weiss
17:15 – 17:35 Studying disks through episodic accretion and variability: exploring the time dimension Aurora Sicilia-Aguilar
17:35 – 17:55 Episodic accretion as time-dependent initial condition for planet-formation Ágnes Kóspál
Oct 11, Tuesday
9:00 – 9:35 Tracing the Ingredients of Habitable Worlds Ted Bergin
9:35 – 9:55 DCO+, DCN, N2D+, and H2CO in the disk of HD163296 Michiel Hogerheijde
9:55 – 10:40 The ice reservoir and snow lines in protoplanetary disks Michiel Min
10:40 – 11:30 coffee break  
11:30 – 12:05 Ice chemistry during the epoch of planet formation Catherine Walsh
12:05 – 12:25 The importance of chemical evolution for setting the volatile composition in
planet-forming regions
Christian Eistrup
12:25 – 14:25 lunch break (optional program at 13:50: visit of the observatory library)  
14:25 – 15:00 Giant planet formation via pebble accretion Bertram Bitsch
15:00 – 15:20 Millimeter-wave polarization of transition disks due to dust scattering Adriana Pohl
15:20 – 15:40 Dust coagulation with porosity evolution Akimasa Kataoka
15:40 – 16:40 coffee break  
16:40 – 17:00 The Heidelberg planetesimal factory Til Birnstiel
15:00 – 17:20 Spirals, gaps and horseshoes in protoplanetary discs Giovanni Dipierro
17:20 – 17:40 Vortex-aided planet formation Zsolt Regály
Oct 12, Wednesday
9:00 – 9:35 Vertical transport of dust, ice, and water in planet-forming regions Sebastiaan Krijt
9:35 – 10:10 Linking the Formation History of Planets with their Spectrum Christoph Mordasini
10:10 – 10:30 How the circumplanetary disk affects the observability of the young, accreting planets? Judit Szulágyi
10:30 – 11:30 coffee break  
11:30 – 11:50 Characterization of planetary systems during the SHINE/SPHERE direct imaging survey Mickael Bonnefoy
11:50 – 12:25 Diverse clouds in chemically diverse planetary atmospheres Christiane Helling
12:25 – 14:25 lunch break (optional program at 13:50: visit of the telescope in the observatory garden)  
14:25 – 14:45 Composition and the mass-radius relation of exoplanets Allona Vazan
14:45 – 15:20 How to design a planetary system for different scattering outcomes Mark Wyatt
15:20 – 15:40 ALMA observations of HD 181327 and Eta Corvi debris discs Sebastian Marino
15:40 – 16:40 coffee break  
16:40 – 17:00 New ALMA observations of the beta Pictoris disk: exocometary gas and dust from
outward migration of beta Pic c
Luca Matrà
17:00 – 17:20 Evolution of gas in debris discs, towards understanding observations Quentin Kral
17:20 – 17:40 Self-stirring in young spatially resolved debris disks Attila Moór
~19:00 Conference dinner (at Rudas bath)  
Oct 13, Thursday
9:00 – 9:35 Heat sources in early planetesimals Ákos Kereszturi
9:35 – 9:55 Searching for biosignatures in exoplanetary impact ejecta Gianni Cataldi
9:55 – 10:15 Testing the formation paradigm of differentiated planetesimals in the Solar System Dagmara Oszkiewicz
10:15 – 11:15 coffee break  
11:15 – 11:50 Collision history of the Kuiper belt and binary Kuiper belt objects Csaba Kiss
11:50 - 12:25 Closing remarks Edwin Bergin
12:25 – 14:25 lunch break  
~15:00 Social program (boat trip on the Danube)