Cernicharo, J.; Goicoechea, J. R.; Daniel, F.; Agúndez, M.; Caux, E.; de Graauw, T.; De Jonge, A.; Kester, D.; Leduc, H. G.; Steinmetz, E.et al.; Stutzki, J.; Ward, J. S.: The 35CI/37CI isotopic ratio in dense molecular clouds: HIFI obervations of hydrogen chloride towards W3 A*. Astronomy and Astrophysics 518, L115 (2010)
Joblin, C.; Pilleri, P.; Montillaud, J.; Fuente, A.; Gerin, M.; Berné, O.; Ossenkopf, V.; Le Bourlot, J.; Teyssier, D.; Goicoechea, J. R.et al.; Le Petit, F.; Röllig, M.; Akyilmaz, M.; Benz, A. O.; Boulanger, F.; Bruderer, S.; Dedes, C.; France, K.; Güsten, R.; Harris, A.; Klein, T.; Kramer, C.; Lord, S. D.; Martin, P. G.; Martin-Pintado, J.; Mookerjea, B.; Okada, Y.; Phillips, T. G.; Rizzo, J. R.; Simon, R.; Stutzki, J.; van der Tak, F.; Yorke, H. W.; Steinmetz, E.; Jarchow, C.; Hartogh, P.; Honingh, C. E.; Siebertz, O.; Caux, E.; Colin, B.: Gas morphology and energetics at the surface of PDRs: New insights with Herschel observations of NGC 7023. Astronomy and Astrophysics 521, L25 (2010)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
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.