Konferenzen zum Thema Astronomie, Astrophysik und Kosmologie in der Tschechischen Republik

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1
Wheel of Star Formation
20. Sep 2021 - 24. Sep 2021 • Prag, Tschechische Republik
Zusammenfassung:
The Physics of Galaxies research group is a part of the Galaxies and Planetary Systems department of the Astronomical Institute of the Czech Academy of Sciences. Our studies use our own observations spanning radio, millimetre and optical wavelengths from the VLA, Arecibo, ALMA and various ESO telescopes, complemented with existing archival data. We also perform numerical N-body and hydrodynamical simulations using the facilities of the Astronomical Institute and on supercomputers elsewhere.
Themen:
Postponed to 12th - 16th September 2022
Eintrags-ID:
1409113
2
Texas2021 — 31st Texas Symposium on Relativistic Astrophysics
13. Dez 2021 - 17. Dez 2021 • Prag, Tschechische Republik
Veranstalter:
Astronomical Institute od the Czech Academy of Sciences
Zusammenfassung:
Since 1978, the Texas Symposium has the tradition of moving around the globe and taking place at various cities. Bohemia (Czech Republic) has always had a rich history in the context of physics, astronomy, and gravitation theory with names of Kepler, Doppler, Mach, Einstein and others having made their discoveries there. In 2021, this historic tradition will be complemented by a Texas Symposium coming to Prague, the country's capital.
Kontakt:
Conference secretariat;     Email: info@texas2021.org
Themen:
gravity, cosmology, gravitational waves, relativity
Eintrags-ID:
1414784
3
Janfest 2022: Wheel of Star Formation — A conference dedicated to Prof. Jan Palouš
12. Sep 2022 - 16. Sep 2022 • Prag, Tschechische Republik
Zusammenfassung:
In light of the COVID-19 outbreak, we decided to postpone the Wheel of Star Formation conference that was originally planned to take place in Prague in September 2020.

The Physics of Galaxies research group is a part of the Galaxies and Planetary Systems department of the Astronomical Institute of the Czech Academy of Sciences. Our studies use our own observations spanning radio, millimetre and optical wavelengths from the VLA, Arecibo, ALMA and various ESO telescopes, complemented with existing archival data. We also perform numerical N-body and hydrodynamical simulations using the facilities of the Astronomical Institute and on supercomputers elsewhere.

Eintrags-ID:
1429200


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Stand vom 05. Juni 2021