Boattini, A.; D'Abramo, G.; Scholl, G.; Hainaut, H.; Boehnhardt, H.; West, R.; Carpino, M.; Hahn, G.; Michelsen, R.; Forti, G.et al.; Pravec, P.; Valsecchi, G. P.; Asher, D. J.: Near-Earth asteroid search and follow-up beyond the 22nd magnitude: A pilot program with ESO telescopes. Astronomy and Astrophysics 418, pp. 743 - 750 (2004)
de Bergh, C.; Boehnhardt, H.; Barucci, A.; Lazzarin, A.; Fornasier, S.; Romon-Martin, J.; Tozzi, G. P.; Doressoundiram, A.; Dotto, E.: Aqueous altered silicates at the surface of two Plutinos? Astronomy and Astrophysics 416, pp. 791 - 798 (2004)
Delsanti, A.; Hainaut, O.; Jourddeuil, E.; Meech, K. J.; Boehnhardt, H.; Barrera, L.: Simultaneous visible and near-IR photometric study of Kuiper Belt Object surfaces with the ESO Very Large Telescopes. Astronomy and Astrophysics 417, pp. 1145 - 1158 (2004)
Fornasier, S.; Doressoundiram, A.; Tozzi, G. P.; Barucci, A.; Boehnhardt, H.; de Bergh, C.; Delsanti, A.; Davies, J.; Dotto, E.: ESO Large Program on physical studies of Transneptunian Objects and Centaurs: Final results of the visible spectrophotometric observations. Astronomy and Astrophysics 421, pp. 353 - 363 (2004)
Lara, L. M.; Rodrigo, R.; Tozzi, G. P.; Boehnhardt, H.; Leisy, P.: The spectrum of Comet C/1999 H1 (Lee) between 0.6 and 1 micron. Astronomy and Astrophysics 420, pp. 371 - 382 (2004)
Lara, L. M.; Tozzi, G. P.; Boehnhardt, H.; D'Martino, M.; Schulz, R.: Gas and Dust in Comet C/2000 WM1 during its closest approach to Earth: Optical imaging and long-slit spectroscopy. Astronomy and Astrophysics 422, pp. 717 - 729 (2004)
Schulz, R.; Stüwe, J. A.; Boehnhardt, H.: Rosetta target Comet 67P/Churyumov-Gerasimenko: Post-perihelion gas and dust production rates. Astronomy and Astrophysics 422 (1), pp. L19 - L21 (2004)
Schütz, O.; Boehnhardt, H.; Pantin, E.; Sterzik, M.; Els, S.; Hahn, J.; Henning, T.: A search for circumstellar dust disks with ADONIS. Astronomy and Astrophysics 424, pp. 613 - 618 (2004)
Tozzi, G. P.; Lara, L. M.; Kolokolova, L.; Boehnhardt, H.; Licandro, J.; Schulz, R.: Sublimating components in the coma of Comet C/2000 WM1 (LINEAR). Astronomy and Astrophysics 424, pp. 325 - 330 (2004)
Schulz, R.; Alexander, C.; Boehnhardt, H.; Glassmeier, K.-H. (Eds.): Rosetta-ESA's Mission to the Origin of the Solar System. Springer Press, Heidelberg (2009)
Barucci, M. A.; Boehnhardt, H.; Cruikshank, D. P.; Morbidelli, A. (Eds.): The Solar System Beyond Neptune. University of Arizona Press, Tucson, USA (2008)
Boehnhardt, H.: Die Planeten und ihre Monde. In: Abriss der Astronomie, pp. 104 - 128 (Eds. Röser, H.-J.; Tscharnuter, W.). Wiley-VCH Verlag, Berlin (2012)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".