| 4.3.2020 |
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Petr Fatka (Astronomical Institute of the Czech Academy of Sciences, Ondřejov; Astronomical Institute of Charles University, Prague)
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Asteroid pairs and clusters
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| 26.2.2020 |
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Olga Maryeva (Astronomical Institute of the Czech Academy of Sciences, Ondřejov)
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Romano's star - why we continue to study it
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| 19.2.2020 |
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Peter Boorman (Astronomical Institute of the Czech Academy of Sciences, Prague)
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Finding hungry supermassive black holes
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| 8.1.2020 |
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Jaroslav Urbář (Ústav fyziky atmosféry Akademie věd České republiky, Praha)
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Příležitosti (nejen) v projektech Planetary Defence programu Space Safety Evropské kosmické agentury
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| 18.12.2019 |
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Jiří Grygar (Fyzikální ústav Akademie věd České republiky, Praha)
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Žeň objevů 2018
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| 11.12.2019 |
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Petr Harmanec (Astronomický ústav UK, Praha)
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Závod o dobytí Měsíce 1957-1970
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| 4.12.2019 |
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Anna Lisa Varri (University of Edinburgh, UK)
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The new phase space complexity of old globular clusters
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| 27.11.2019 |
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František Dinnbier (University of Cologne, Germany)
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Tidal tails of open star clusters as probes to early gas expulsion: predictions for Gaia
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| 20.11.2019 |
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Martin Šolc (Astronomický ústav UK, Praha)
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Johannes Kepler a jeho 3. zákon (1619)
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| 13.11.2019 |
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Robin Eappen (Astronomical Institute of Charles University, Prague)
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FatController: an application of CLMASS package to XMM Cluster Survey
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| 6.11.2019 |
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Josef Hanuš, Miroslav Brož, Pavel Ševeček (Astronomical Institute of Charles University, Prague)
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Do we have another dwarf planet in the main belt?
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| 30.10.2019 |
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Nadia Blagorodnova (Radboud University, Nijmegen, Netherlands)
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Observational study of common-envelope transients: the final stellar dance
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| 23.10.2019 |
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Jan Pflamm-Altenburg (University of Bonn, Germany)
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Regularisation of few-body dynamics
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| 16.10.2019 |
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Marie Karjalainen (Instituto de Astrofísica de Canarias, Tenerife, Spain)
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A planet search among Kepler giant stars
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| 9.10.2019 |
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Petr Kubánek (Large Binocular Telescope Observatory, Arizona, USA)
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Astronomy and software engineering
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| 2.10.2019 |
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Pavel Kroupa (University of Bonn, Germany; Astronomical Institute of Charles University, Prague)
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The systematically varying stellar initial mass function and some implications thereof
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