Zobrazeno 1 - 10
of 365
pro vyhledávání: '"Castillo‐Rogez, J."'
Autor:
Landis, M. E., Byrne, S., Schörghofer, N., Schmidt, B. E., Hayne, P. O., Castillo-Rogez, J., Sykes, M. V., Combe, J.-P., Ermakov, A. I., Prettyman, T. H., Raymond, C. A., Russell, C. T.
Observations of a water vapor exosphere around Ceres suggest that the dwarf planet may be episodically outgassing at a rate of similar to 6 kg s(-1) from unknown sources. With data from the Dawn mission as constraints, we use a coupled thermal and va
Externí odkaz:
http://hdl.handle.net/10150/626274
http://arizona.openrepository.com/arizona/handle/10150/626274
http://arizona.openrepository.com/arizona/handle/10150/626274
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
Publikováno v:
Monthly Notices of the Royal Astronomical Society Main Journal, 2020
Ceres is the largest body in the Main Belt, and it is characterized by a large abundance of water ice in its interior. This feature is suggested by its relatively low bulk density (2162 kg m$^{-3}$), while its partial differentiation into a rocky cor
Externí odkaz:
http://arxiv.org/abs/2004.10504
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
Akademický článek
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Autor:
Belov, K., Branch, A., Broschart, S., Castillo-Rogez, J., Chien, S., Clare, L., Dengler, R., Gao, J., Garza, D., Hegedus, A., Hernandez, S., Herzig, S., Imken, T., Kim, H., Mandutianu, S., Romero-Wolf, A., Schaffer, S., Troesch, M., Wyatt, E. J., Lazio, J.
Publikováno v:
Exp Astron (2018) 46: 241
This paper reports a design study for a space-based decametric wavelength telescope. While not a new concept, this design study focused on many of the operational aspects that would be required for an actual mission. This design optimized the number
Externí odkaz:
http://arxiv.org/abs/1904.00119
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