Zobrazeno 1 - 10
of 185
pro vyhledávání: '"Kramm, U."'
Autor:
Lausch, M., Zimina, A., Bao, J., Pashminehazar, R., Etzold, B. J. M., Kramm, U. I., Grunwaldt, J.-D., Hussong, J.
Publikováno v:
Journal of Chemical Physics; 11/21/2024, Vol. 161 Issue 19, p1-34, 34p
Autor:
Maciejewski, G., Niedzielski, A., Wolszczan, A., Nowak, G., Neuhaeuser, R., Winn, J. N., Deka, B., Adamów, M., Górecka, M., Fernandez, M., Aceituno, F. J., Ohlert, J., Errmann, R., Seeliger, M., Dimitrov, D., Latham, D. W., Esquerdo, G. A., McKnight, L., Holman, M. J., Jensen, E. L. N., Kramm, U., Pribulla, T., Raetz, St., Schmidt, T. O. B., Ginski, Ch., Mottola, S., Hellmich, S., Adam, Ch., Gilbert, H., Mugrauer, M., Saral, G., Popov, V., Raetz, M.
There have been previous hints that the transiting planet WASP-3 b is accompanied by a second planet in a nearby orbit, based on small deviations from strict periodicity of the observed transits. Here we present 17 precise radial velocity measurement
Externí odkaz:
http://arxiv.org/abs/1309.6733
Transit and radial velocity observations continuously discover an increasing number of exoplanets. However, when it comes to the composition of the observed planets the data are compatible with several interior structure models. Thus, a planetary par
Externí odkaz:
http://arxiv.org/abs/1112.2087
Autor:
Neuhäuser, R., Errmann, R., Berndt, A., Maciejewski, G., Takahashi, H., Chen, W. P., Dimitrov, D. P., Pribulla, T., Nikogossian, E. H., Jensen, E. L. N., Marschall, L., Wu, Z. -Y., Kellerer, A., Walter, F. M., Briceño, C., Chini, R., Fernandez, M., Raetz, St., Torres, G., Latham, D. W., Quinn, S. N., Niedzielski, A., Bukowiecki, Ł., Nowak, G., Tomov, T., Tachihara, K., Hu, S. C. -L., Hung, L. W., Kjurkchieva, D. P., Radeva, V. S., Mihov, B. M., Slavcheva-Mihova, L., Bozhinova, I. N., Budaj, J., Vaňko, M., Kundra, E., Hambálek, Ľ., Krushevska, V., Movsessian, T., Harutyunyan, H., Downes, J. J., Hernandez, J., Hoffmeister, V. H., Cohen, D. H., Abel, I., Ahmad, R., Chapman, S., Eckert, S., Goodman, J., Guerard, A., Kim, H. M., Koontharana, A., Sokol, J., Trinh, J., Wang, Y., Zhou, X., Redmer, R., Kramm, U., Nettelmann, N., Mugrauer, M., Schmidt, J., Moualla, M., Ginski, C., Marka, C., Adam, C., Seeliger, M., Baar, S., Roell, T., Schmidt, T. O. B., Trepl, L., Eisenbeiß, T., Fiedler, S., Tetzlaff, N., Schmidt, E., Hohle, M. M., Kitze, M., Chakrova, N., Gräfe, C., Schreyer, K., Hambaryan, V. V., Broeg, C. H., Koppenhoefer, J., Pandey, A. K.
We present the Young Exoplanet Transit Initiative (YETI), in which we use several 0.2 to 2.6m telescopes around the world to monitor continuously young (< 100 Myr), nearby (< 1 kpc) stellar clusters mainly to detect young transiting planets (and to s
Externí odkaz:
http://arxiv.org/abs/1106.4244
Publikováno v:
A&A, 2011
In order to accurately model giant planets, a whole set of observational constraints is needed. As the conventional constraints for extrasolar planets like mass, radius, and temperature allow for a large number of acceptable models, a new planetary p
Externí odkaz:
http://arxiv.org/abs/1101.0997
Photometric follow-ups of transiting exoplanets (TEPs) may lead to discoveries of additional, less massive bodies in extrasolar systems. This is possible by detecting and then analysing variations in transit timing of transiting exoplanets. In 2009 w
Externí odkaz:
http://arxiv.org/abs/1010.3122
Autor:
Maciejewski, G., Neuhaeuser, R., Errmann, R., Mugrauer, M., Adam, Ch., Berndt, A., Eisenbeiss, T., Fiedler, S., Ginski, Ch., Hohle, M., Kramm, U., Marka, C., Moualla, M., Pribulla, T., Raetz, St., Roell, T., Schmidt, T. O. B., Seeliger, M., Spaleniak, I., Tetzlaff, N., Trepl, L.
Transiting exoplanets (TEPs) observed just about 10 Myrs after formation of their host systems may serve as the Rosetta Stone for planet formation theories. They would give strong constraints on several aspects of planet formation, e.g. time-scales (
Externí odkaz:
http://arxiv.org/abs/1010.3118
The planet GJ 1214b is the second known super-Earth with a measured mass and radius. Orbiting a quiet M-star, it receives considerably less mass-loss driving X-ray and UV radiation than CoRoT-7b, so that the interior may be quite dissimilar in compos
Externí odkaz:
http://arxiv.org/abs/1010.0277
GJ 436b is the first extrasolar planet discovered that resembles Neptune in mass and radius. The particularly interesting property of Neptune-sized planets is that their mass Mp and radius Rp are close to theoretical M-R relations of water planets. G
Externí odkaz:
http://arxiv.org/abs/1002.4447
Publikováno v:
International Journal of Earth Sciences. Nov2017, Vol. 106 Issue 8, p2797-2813. 17p.