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FG 1 The physics underpinning multi-scale, spatially-resolved star formation relations Convenors: Diederik Kruijssen, Andi Burkert Chair: Markus Nielbock |
| 11:20-11:35 | Andi Burkert | Introduction |
| 11:35-11:45 | Paolo Padoan | The role and the origin of the virial parameter |
| 11:45-11:55 | Sergio Molinari | Characterising basic ingredients for a bottom-up Galaxy-scale SF recipe |
| 11:55-12:05 | Rowan Smith | Molecular Cloud Environments from Galactic Scale Simulations |
| 12:05-12:10 | Diederik Kruijssen | An uncertainty principle for star formation |
| 12:10-12:40 | Discussion | |
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FG 2 Characterizing cloud structure in observations and simulations Convenors: Thomas Robitaille, Adam Ginsburg Chair: Juergen Steinacker |
| 11:20-11:30 | Thomas Robitaille | Introduction |
| 11:30-11:38 | Clare Dobbs | Large scale HI and CO maps from simulations and observations |
| 11:38-11:46 | Anna McLeod | Extracting observables from simulations of star forming clouds including stellar feedback |
| 11:46-11:54 | Josep Girart | Magnetic fields from large to small scales: How can we connect them? |
| 11:54-12:02 | Alvaro Hacar | Friends-In-VElocity - A filament-finding tool |
| 12:02-12:10 | Ke Wang | Hierarchical Structures and Kinematics of a 30 pc IR-dark Filament |
| 12:10-12:40 | Discussion | |
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FG 3 A Comparison of star formation in the Galactic center and the Galactic disk> Convenor: Eric Keto Chair: Hendrik Linz |
| 14:00-14:16 | Eric Keto | Introduction |
| 14:16-14:25 | Adam Ginsburg | A comparison of cm-wavelength H2CO observations in the CMZ (specifically, the Brick) vs. in W51 |
| 14:25-14:34 | Katharine Johnston | The structure and star-forming fate of the Galactic centre cloud G0.253+0.016 |
| 14:34-14:43 | Christine Koepferl | The Star-formation Rate of the Central Molecular Zone determined from Young Stellar Objects |
| 14:43-14:52 | Diederik Kruijssen | The extreme environment of the CMZ: suppressed star formation and an absolute-time sequence of star-forming clouds |
| 14:52-15:20 | Discussion | |
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FG 4 Interstellar Turbulence as a Bridge Connecting Large and Small Scale Processes Convenors: Alexei Kritsuk, Andi Burkert Chair: Sarah Ragan |
| 14:00-14:15 | Alexei Kritsuk | Introduction |
| 14:15-14:25 | Diederik Kruijssen | Turbulence in high-pressure environments: the Galactic centre and high-redshift galaxies |
| 14:25-14:35 | Chat Hull | Does turbulence cause the misalignment of outflows and magnetic fields in protostellar cores? |
| 14:35-14:45 | Juergen Steinacker | The puzzle of connecting filament-scale turbulence and core center turbulence |
| 14:45-14:55 | Paolo Padoan | Inertial-range statistics of SN-driven turbulence |
| 14:55-15:20 | Discussion | |
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The EPoS way: Large group, small room, remote location. Consider all aspects.
Short talks, intense discussions. |