Krüger, H.: Rosetta - Rendezvous mit einem Kometen. Vortragsreihe "Raumfahrt aus Leidenschaft'' an der Universität Stuttgart, Institut für Raumfahrtsysteme, Stuttgart (2014)
Krüger, H.; The SESAME Team: Grain Properties at the Nucleus of Comet 67P/C-G. 37th Rosetta Science Working Team Meeting, Villafranca del Castillo, Spain (2014)
Krüger, H.; Altobelli, N.; Strub, P.; Sterken, V.; Srama, R.; Grün, E.: Interstellar Dust in the Solar System: Model versus In-Situ Spacecraft Data. European Geophysical Union General Assembly, Vienna, Austria (2019)
Boehnhardt, H.; Krueger, H.; Mall, U.: Assessing the Primordial Character of Comets and of 67P/Churyumov-Gerasimenko. 50th ESLAB Symposium 2016, Leiden, Netherlands (2016)
Jockers, K.; Boehnhardt, H.; Krueger, H.; Mall, U.: Assessing the Primordial Character of Comets and of 67P/Churyumov-Gerasimenko. COMETS 2016, Toulouse, France (2016)
A star’s chemical composition strongly influences the ultraviolet radiation it emits into space and thus the conditions for the emergence of life in its neighbourhood.
A single star has provided information about the collision of the Milky Way with the dwarf galaxy Gaia-Enceladus. The event likely took place approximately 11.5 billion years ago.