Zobrazeno 1 - 10
of 531
pro vyhledávání: '"Witasse O"'
Autor:
Huybrighs, H. L. F., Roussos, E., Blöcker, A., Krupp, N., Futaana, Y., Barabash, S., Hadid, L. Z., Holmberg, M. K. G., Witasse, O.
In Huybrighs et al., 2020 we investigated energetic proton depletions along Galileo's Europa flyby E26. Based on a particle tracing analysis we proposed that depletions are caused by perturbed electrogmagnetic fields combined with atmospheric charge
Externí odkaz:
http://arxiv.org/abs/2108.10255
Autor:
Marchis, F., Jorda, L., Vernazza, P., Brož, M., Hanuš, J., Ferrais, M., Vachier, F., Rambaux, N., Marsset, M., Viikinkoski, M., Jehin, E., Benseguane, S., Podlewska-Gaca, E., Carry, B., Drouard, A., Fauvaud, S., Birlan, M., Berthier, J., Bartczak, P., Dumas, C., Dudzinski, G., Durech, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Fetick, R., Fusco, T., Grice, J., Kryszczynska, A., Lamy, P., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Santana-Ros, T., Tanga, P., Vigan, A., Witasse, O., Yang, B.
Publikováno v:
A&A 653, A57 (2021)
Context. The recent estimates of the 3D shape of the M/Xe-type triple asteroid system (216) Kleopatra indicated a density of 5 g.cm$^{-3}$. Such a high density implies a high metal content and a low porosity which is not easy to reconcile with its pe
Externí odkaz:
http://arxiv.org/abs/2108.07207
Autor:
Brož, M., Marchis, F., Jorda, L., Hanuš, J., Vernazza, P., Ferrais, M., Vachier, F., Rambaux, N., Marsset, M., Viikinkoski, M., Jehin, E., Benseguane, S., Podlewska-Gaca, E., Carry, B., Drouard, A., Fauvaud, S., Birlan, M., Berthier, J., Bartczak, P., Dumas, C., Dudziński, G., Ďurech, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Fetick, R., Fusco, T., Grice, J., Kryszczynska, A., Lamy, P., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Santana-Ros, T., Tanga, P., Vigan, A., Vokrouhlický, D., Witasse, O., Yang, B.
Publikováno v:
A&A 653, A56 (2021)
To interpret adaptive-optics observations of (216) Kleopatra, we need to describe an evolution of multiple moons, orbiting an extremely irregular body and including their mutual interactions. Such orbits are generally non-Keplerian and orbital elemen
Externí odkaz:
http://arxiv.org/abs/2105.09134
Autor:
Carry, B., Vernazza, P., Vachier, F., Neveu, M., Hanus, J. Berthier J., Ferrais, M., Jorda, L., Marsset, M., Viikinkoski, M., Bartczak, P., Behrend, R., Benkhaldoun, Z., Birlan, M., Castillo-Rogez, J., Cipriani, F., Colas, F., Drouard, A., Dudzinski, G. P., Desmars, J., Dumas, C., Durech, J., Fetick, R., Fusco, T., Grice, J., Jehin, E., Kaasalainen, M., Kryszczynska, A., Lamy, P., Marchis, F., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Podlewska-Gaca, E., Rambaux, N., Santana-Ros, T., Storrs, A., Tanga, P., Vigan, A., Warner, B., Wieczorek, M., Witasse, O., Yang, B.
Publikováno v:
A&A 650, A129 (2021)
Dynamical models of Solar System evolution have suggested that P-/D-type volatile-rich asteroids formed in the outer Solar System and may be genetically related to the Jupiter Trojans, the comets and small KBOs. Indeed, their spectral properties rese
Externí odkaz:
http://arxiv.org/abs/2103.06349
Autor:
Yang, B., Hanus, J., Carry, B., Vernazza, P., Broz, M., Vachier, F., Rambaux, N., Marsset, M., Chrenko, O., Sevecek, P., Viikinkoski, M., Jehin, E., Ferrais, M., Gaca, E. Podlewska, Drouard, A., Marchis, F., Birlan, M., Benkhaldoun, Z., Berthier, J., Bartczak, P., Dumas, C., Dudzinski, G., Durech, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Fetick, R., Fusco, T., Grice, J., Jorda, L., Kaasalainen, M., Kryszczynska, A., Lamy, P., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Santana-Ros, T., Tanga, P., Vigan, A., Witasse, O.
Publikováno v:
A&A 641, A80 (2020)
Asteroid (31) Euphrosyne is one of the biggest objects in the asteroid main belt and the Euphrosyne family occupies a highly inclined region in the outer main belt and contains a remarkably large number of members, which is interpreted as an outcome
Externí odkaz:
http://arxiv.org/abs/2007.08059
Autor:
Wörner, L., Root, B.C., Bouyer, P., Braxmaier, C., Dirkx, D., Encarnação, J., Hauber, E., Hussmann, H., Karatekin, Ö., Koch, A., Kumanchik, L., Migliaccio, F., Reguzzoni, M., Ritter, B., Schilling, M., Schubert, C., Thieulot, C., Klitzing, W.v., Witasse, O.
Publikováno v:
In Planetary and Space Science December 2023 239
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Autor:
Hanuš, J., Vernazza, P., Viikinkoski, M., Ferrais, M., Rambaux, N., Podlewska-Gaca, E., Drouard, A., Jorda, L., Jehin, E., Carry, B., Marsset, M., Marchis, F., Warner, B., Behrend, R., Asenjo, V., Berger, N., Bronikowska, M., Brothers, T., Charbonnel, S., Colazo, C., Coliac, J-F., Duffard, R., Jones, A., Leroy, A., Marciniak, A., Melia, R., Molina, D., Nadolny, J., Person, M., Pejcha, O., Riemis, H., Shappee, B., Sobkowiak, K., Soldán, F., Suys, D., Szakats, R., Vantomme, J., Birlan, M., Berthier, J., Bartczak, P., Dumas, C., Dudziński, G., Ďurech, J., Castillo-Rogez, J., Cipriani, F., Fetick, R., Fusco, T., Grice, J., Kaasalainen, M., Kryszczynska, A., Lamy, P., Michalowski, T., Michel, P., Santana-Ros, T., Tanga, P., Vachier, F., Vigan, A., Witasse, O., Yang, B.
Publikováno v:
A&A 633, A65 (2020)
With an estimated diameter in the 320 to 350 km range, (704) Interamnia is the fifth largest main belt asteroid and one of the few bodies that fills the gap in size between the four largest bodies with $D$ > 400 km (Ceres, Vesta, Pallas and Hygiea) a
Externí odkaz:
http://arxiv.org/abs/1911.13049
Autor:
Peter, Kerstin, Pätzold, M., Montabone, L., Thiemann, E., González-Galindo, F., Witasse, O., Tellmann, S., Bird, M.K.
Publikováno v:
In Icarus August 2023 400
Autor:
Hanuš, J., Marsset, M., Vernazza, P., Viikinkoski, M., Drouard, A., Brož, M., Carry, B., Fetick, R., Marchis, F., Jorda, L., Fusco, T., Birlan, M., Santana-Ros, T., Podlewska-Gaca, E., Jehin, E., Ferrais, M., Grice, J., Bartczak, P., Berthier, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Dudzinski, G., Dumas, C., Ďurech, J., Kaasalainen, M., Kryszczynska, A., Lamy, P., Coroller, H. Le, Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Tanga, P., Vachier, F., Vigan, A., Witasse, O., Yang, B.
Publikováno v:
A&A 624, A121 (2019)
Asteroid (7) Iris is an ideal target for disk-resolved imaging owing to its brightness (V$\sim$7-8) and large angular size of 0.33 arcsec during its apparitions. Iris is believed to belong to the category of large unfragmented asteroids that avoided
Externí odkaz:
http://arxiv.org/abs/1902.09242