Rengel, M.; Hartogh, P.; Jarchow, C.: HHSMT observations of the Venusian mesospheric temperature, winds, and CO abundance around the MESSENGER flyby. Planetary and Space Science 56, pp. 1688 - 1695 (2008)
Rengel, M.; Hartogh, P.; Jarchow, C.: Mesospheric vertical thermal structure and winds on Venus from HHSMT CO spectral-line observations. Planetary and Space Science 56, pp. 1368 - 1384 (2008)
Tachihara, K.; Rengel, M.; Nakajima, Y.; Yamaguchi, N.; André, P.; Neuhäuser, R.; Onishi, T.; Fukui, Y.; Mizuno, A.: Gas and Dust Condensations and a Peculiar Class 0 Object in the Lupus 3 Star-Forming Cloud. Astrophysical Journal 659, pp. 1382 - 1393 (2007)
Limaye, S.; Rengel, M.: 5 - Atmospheric circulation and dynamics - Observations and knowledge gaps. In: Towards understanding the climate of Venus: Applications of terrestrial models to our sister planet, pp. 55 - 72 (Eds. Bengtsson, L.; Bonnet, R.-M.; Grinspoon, D.; Koumoutsaris, S.; Lebonnois, S. et al.). Springer-Verlag, Berlin (2012)
Rengel, M.; Sagawa, H.; Hartogh, P.: Retrieval Simulations of Atmospheric Gases from Herschel observations of Titan. In: Advances in Geosciences, pp. 335 - 348 (Eds. Bhardwaj, A.; Haider, S. A.; Hartogh, P.; Ip, W.-H.; Ito, T. et al.). World Scientific Publishing Co., Singapore (2011)
Rengel, M.; Küppers, M.; Keller, H. U.; Gutierrez, P.: Modeling of the Terminal Velocities of the Dust Ejected Material by the Impact. In: Deep Impact as a World Observatory Event - Synergies in Space, Time (Eds. Kaeufl, H. U.; Sterken, C.). Springer Verlag (2007)
Soderblom, D. R.; Nave, G. (Eds.): About the atomic and molecular databases in the planetary community - A contribution in the Laboratory Astrophysics Data WG IAU 2022 GA session. IAU Symposium, 2024. (2024), 87-91 pp.
de Val-Borro, M.; Hartogh, P.; Jarchow, C.; Rengel, M.; Villanueva, G. L.; Küppers, M.; Biver, M.; Bockelée-Morvan, D.; Crovisier, J.: The volatile composition of comet C/2004 Q2 (Machholz) derived from submillimeter observations. In: Highlights of Spanish Astrophysics VII, Proceedings of the X Scientific Meeting of the Spanish Astronomical Society (SEA) (Eds. Guirado, J. C.; Lara, L. M.; Quilis, V.; Gorgas, J.). (2013)
Küppers, M.; Keller, H. U.; Fornasier, S.; Gutierrez, P.; Hviid, S. F.; Jorda, L.; Knollenberg, J.; Lowry, S. C.; Rengel, M.: Observations of Comet 9P/Tempel 1 and Deep Impact by the OSIRIS Cameras onboard Rosetta. In: Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength, pp. 29 - 39. Springer Berlin / Heidelberg (2009)
Rengel, M.; Küppers, M.; Keller, H. U.; Gutierrez, P.: Modeling of the Terminal Velocities of the Dust Ejected Material by the Impact. In: Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength, pp. 137 - 142. Springer Berlin / Heidelberg (2009)
Rengel, M.; Küppers, M.; Keller, H. U.; Gutierrez, P.; Hviid, S.: The terminal Velocity of the Deep Impact dust Ejecta. In: Revista Mexicana de Astronomía y Astrofísica (SC)., pp. 25 - 26 (Eds. Magris, G.; Bruzual, G.; Carigi, L.). (2009)
Rengel, M.; Hodapp, K.; Eisloeffel, J.: SK 1: A Possible Case of Triggered Star Formation in Perseus. In: Triggered Star Formation in a Turbulent Interstellar Medium (IAU S237) (Eds. Elmegreen, B.; Palous, J.). Cambridge University Press (2007)
Rengel, M.; Froebrich, D.; Eislöffel, J.; Hodapp, K.: Submillimetre Imaging of Deeply Embedded Outflow Sources and Class 0 Sources. In: Abstracts of Contributed Talks and Posters presented at the Annual Scientific Meeting of the Astronomische Gesellschaft at the Joint European and National Meeting JENAM 2001. (2001)
Rengel, M.: Caracterizando las atmósferas de los planetas: espectros, procesos y estructura. BrainGain-PWF Venezuelan Physics School 2022, Online (2022)
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
Studies of the Sun or other stars rely on indirect observations, i.e. we can only observe effects of an unknown quantity. This group works on the corresponding inverse problem to reconstruct the unknown cause from the observed effect, e.g. the reconstruction of convection fields from measurements of oscillations of the solar surface.