Strub, P.; Krüger, H.; Sterken, V. J.: Sixteen Years of Ulysses Interstellar Dust Measurements in the Solar System. II. Fluctuations in the Dust Flow from the Data. Astrophysical Journal 812, pp. 140 - 154 (2015)
Hornung, K.; Kissel, J.; Fischer, H.; Mellado, E. M.; Kulikov, O.; Hilchenbach, M.; Krüger, H.; Engrand, C.; Langevin Yves Massimiliano Rossi a, F. R. K. e.: Collecting cometary dust particles on metal blacks with the COSIMA instrument onboard ROSETTA. Planetary and Space Science 103, pp. 309 - 317 (2014)
Krüger, H.: Kometen - Kleinkörper aus Eis und Staub; Neue Erkenntnisse der Kometenforschung. Interstellarum Themenheft Kometen (1/2014), pp. 16 - 23 (2014)
Flandes, A.; Krüger, H.; Loose, A.; Sperl, M.; Seidensticker, K. J.; Fischer, H.-H.; Arnold, W.: Dust Impact Monitor (DIM) onboard Rosetta/Philae: Comparison of experimental results and the theory behind the experiment. Planetary and Space Science 84, pp. 122 - 130 (2013)
Soja, R.; Altobelli, N.; Krüger, H.; Sterken, V.: Dust environment prediction for the ESA L-Class mission candidate JUICE. Planetary and Space Science 75, pp. 117 - 128 (2013)
Sterken, V. J.; Altobelli, N.; Kempf, S.; Krüger, H.; Srama, R.; Strub, P.; Gruen, E.: The filtering of interstellar dust in the solar system. Astronomy and Astrophysics 552, A130 (2013)
Krüger, H.: 50 Jahre Planetenforschung - Aus fernen Welten; Teil 2: Die Gasriesen, ihre Monde und die Kleinkörper. Sterne und Weltraum 09/2012, pp. 46 - 56 (2012)
Sterken, V.; Altobelli, N.; Kempf, S.; Krüger, H.; Postberg, F.; Soja, R.; Srama, R.; Grün, E.: An optimum opportunity for interstellar dust measurements by the JUICE mission. Planetary and Space Science 71, pp. 142 - 146 (2012)
Flandes, A.; Krüger, H.; Hamilton, D. P.; Valdés-Galicia, J. F.; Spilker, L.; Caballero, R.: Magnetic field modulated dust streams from Jupiter in interplanetary space. Planetary and Space Science 59, pp. 1455 - 1471 (2011)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.