Embedded Files
Day 1
05 January 2022
05 January 2022
Welcome 9:00 - 9:15
9:15 - 9:55
A Fast and Accurate Method of Radiation Hydrodynamics Calculation and The Importance of Thermodynamics
A Fast and Accurate Method of Radiation Hydrodynamics Calculation and The Importance of Thermodynamics
Shu-ichiro Inutsuka
9:55 - 10:35
Disc fragmentation in the primordial and low metallicity star formation
Disc fragmentation in the primordial and low metallicity star formation
Takashi Hosokawa
Coffee break 10:35 - 11:00
11:00 - 11:40
Gravitational fragmentation of circumstellar disks in sub-solar metallicity environments
Gravitational fragmentation of circumstellar disks in sub-solar metallicity environments
Eduard Vorobyov
11:40 - 12:20
The properties of protoplanets formed by disc fragmentation
The properties of protoplanets formed by disc fragmentation
Dimitris Stamatellos
Lunch 12:20 - 13:50
Tribute to Willy Kley 13:50 - 14:00
14:00 - 14:40
On the numerics of disk fragmentation: Coordinate systems, sink particle methods, proper convergence, and other bedeviled details
On the numerics of disk fragmentation: Coordinate systems, sink particle methods, proper convergence, and other bedeviled details
Rolf Kuiper
14:40 - 15:10
From disc fragments to companion stars: high resolution modelling of disc fragmentation around forming massive stars
From disc fragments to companion stars: high resolution modelling of disc fragmentation around forming massive stars
Andre Oliva
15:10 - 15:50
Predicting fragmentation in protostellar disks using new theoretical insights on disk evolution
Predicting fragmentation in protostellar disks using new theoretical insights on disk evolution
Wenrui Xu
Day 2
06 January 2022
06 January 2022
9:00 - 9:40
What we know and don’t know about disc GI
What we know and don’t know about disc GI
Sergei Nayakshin
9:40 - 10:40
Disc GI and clump evolution in planet formation
Disc GI and clump evolution in planet formation
Discussion
Coffee break 10:40 - 11:10
11:10 - 11:50
The influence of binary companion on disc fragmentation
The influence of binary companion on disc fragmentation
Ken Rice
11:50 - 12:30
Magnetically controlled disk fragmentation: a new pathway to forming low mass planets around solar mass stars and massive gas giants around massive B stars.
Magnetically controlled disk fragmentation: a new pathway to forming low mass planets around solar mass stars and massive gas giants around massive B stars.
Lucio Mayer
Lunch 12:20 - 14:00
14:00 - 14:40
The burst mode of accretion in massive star formation.
The burst mode of accretion in massive star formation.
Dominique Meyer
14:40 - 15:20
Accretion bursts in high-mass protostars
Accretion bursts in high-mass protostars
Vardan Elbakyan
15:20 - 16:20
Disc GI in star and binary formation
Disc GI in star and binary formation
Discussion(DS)
Day 3
07 January 2022
07 January 2022
9:00 - 10:00
Way forward to simulate and constrain observationally the role of disc GI in star and planet formation
Way forward to simulate and constrain observationally the role of disc GI in star and planet formation
Discussion(SN, AV, RH)
10:00 - 10:30
A condition for self-gravitational fragmentation of protoplanetary discs
A condition for self-gravitational fragmentation of protoplanetary discs
Sanemichi Takahashi
10:30 - 11:00
Investigating disc fragmentation through kinematics
Investigating disc fragmentation through kinematics
Cristiano Longarini
Coffee break 11:00 - 11:30
11:30 - 12:00
DIPSY: A New Disc Instability Population SYnthesis
DIPSY: A New Disc Instability Population SYnthesis
Oliver Schib
12:00 - 12:30
Disc self gravity as a scale for the disc mass
Disc self gravity as a scale for the disc mass
Benedetta Veronesi
Lunch 12:30 - 14:00
14:00 - 14:30
Warping Away Gravitational Instabilities in Protoplanetary Discs
Warping Away Gravitational Instabilities in Protoplanetary Discs
Sahl Rowther
14:30 - 15:30
Concluding remarks
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