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Page 1: PHYSICS AND CHEMISTRY OF STAR FORMATION · Star Formation across Cosmic Time Star Formation across Scales and Environments The ISM and Molecular Clouds: • feedback, quenching, triggering,

The 7th* Chile-Cologne-Bonn-Symposium

PHYSICS AND CHEMISTRY OF STAR FORMATIONTHE DYNAMICAL ISM ACROSS TIME AND SPATIAL SCALES

*in the series of the former Zermatt-Cologne-Bonn Symposia

The conference is co-funded by: CRC 956 (project ID 184018867)

LOCAL ORGANIZING COMMITTEE:

R. Bustos | P. García | N. Gardemann | S. Herbst | W. Max-MoerbeckV. Ossenkopf-Okada | D. Riquelme | R. Rodriguez | Á. Sánchez-MongeR. Schaaf | F. Schlöder | D. Seifried | A. Stutz | J. Stutzki | S. Thorwirth

astro.uni-koeln.de/symposium-star-formation-2020.html

CONTACT: [email protected]

The conference is managed by:Contact: Andrea Lagarini [email protected]

German Research Foundation

September 28 – October 2, 2020Puerto Varas, Chile

Comité Mixto ESO-Chile

SCIENTIFIC ORGANIZING COMMITTEE:

Leo BronfmanScott ChapmanAndrea FerraraJavier GoicoecheaEva SchinnererStephan Schlemmer

Gordon StaceyAmelia StutzSatoko TakahashiEwine van DishoeckJi YangHans Zinnecker

Star Formation across Cosmic TimeStar Formation across Scales and EnvironmentsThe ISM and Molecular Clouds:• feedback, quenching, triggering, turbulence• magnetic fields, fragmentation and collapse, outflows• abundances, chemistry and microphysical processesLaboratory AstrophysicsObservatories and Instrumentation

SESSION TOPICS