Mar 4, 2020 |
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Petr Fatka (Astronomical Institute of the Czech Academy of Sciences, Ondrejov; Astronomical Institute of Charles University, Prague)
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Asteroid pairs and clusters
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Feb 26, 2020 |
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Olga Maryeva (Astronomical Institute of the Czech Academy of Sciences, Ondrejov)
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Romano's star - why we continue to study it
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Feb 19, 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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Jan 8, 2020 |
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Jaroslav Urbar (Ustav fyziky atmosfery Akademie ved Ceske republiky, Praha)
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Prilezitosti (nejen) v projektech Planetary Defence programu Space Safety Evropske kosmicke agentury
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Dec 18, 2019 |
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Jiri Grygar (Fyzikalni ustav Akademie ved Ceske republiky, Praha)
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Zen objevu 2018
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Dec 11, 2019 |
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Petr Harmanec (Astronomicky ustav UK, Praha)
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Zavod o dobyti Mesice 1957-1970
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Dec 4, 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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Nov 27, 2019 |
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Frantisek 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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Nov 20, 2019 |
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Martin Solc (Astronomicky ustav UK, Praha)
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Johannes Kepler a jeho 3. zakon (1619)
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Nov 13, 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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Nov 6, 2019 |
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Josef Hanus, Miroslav Broz, Pavel Sevecek (Astronomical Institute of Charles University, Prague)
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Do we have another dwarf planet in the main belt?
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Oct 30, 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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Oct 23, 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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Oct 16, 2019 |
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Marie Karjalainen (Instituto de Astrofisica de Canarias, Tenerife, Spain)
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A planet search among Kepler giant stars
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Oct 9, 2019 |
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Petr Kubanek (Large Binocular Telescope Observatory, Arizona, USA)
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Astronomy and software engineering
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Oct 2, 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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