Zobrazeno 1 - 10
of 378
pro vyhledávání: '"BIRLAN, M."'
Autor:
Fornasier, S., Dotto, E., Panuzzo, P., Delbò, M., Belskaya, I., Krugly, Y., Inasaridze, R., Barucci, M. A., Perna, D., Brucato, J., Birlan, M.
Publikováno v:
A&A 688, L7 (2024)
This study aims to determine the size, albedo and rotational period of (98943) 2001 CC21, target of the Hayabusa2 extended mission, using thermal data from the Spitzer Space telescope and ground based observations. The Spitzer data were acquired with
Externí odkaz:
http://arxiv.org/abs/2407.13017
Autor:
Brož, M., Vernazza, P., Marsset, M., Binzel, R. P., DeMeo, F., Birlan, M., Colas, F., Anghel, S., Bouley, S., Blanpain, C., Gattacceca, J., Jeanne, S., Jorda, L., Lecubin, J., Malgoyre, A., Steinhausser, A., Vaubaillon, J., Zanda, B.
Publikováno v:
A&A 689, A183 (2024)
The present work aims to determine the source regions of carbonaceous chondrites (CM, CI, CO, CV, CK, CR, CH, CB, or C-ungrouped). We studied 38 individual asteroid families, including young and old ones, and determined their contributions to the NEO
Externí odkaz:
http://arxiv.org/abs/2406.19727
Autor:
Carry, B., Descamps, P., Ferrais, M., Rivet, J. -P., Berthier, J., Jehin, E., Vernet, D., Abe, L., Bendjoya, P., Vachier, F., Pajuelo, M., Birlan, M., Colas, F., Benkhaldoun, Z.
Publikováno v:
A&A 680, A21 (2023)
Every population of small bodies in the Solar system contains a sizable fraction of multiple systems. Among these, the Jupiter Trojans have the lowest number of known binary systems and the least characterized. We aim at characterizing the reported b
Externí odkaz:
http://arxiv.org/abs/2309.15537
Autor:
Hromakina, T., Birlan, M., Barucci, M. A., Fulchignoni, M., Colas, F., Fornasier, S., Merlin, F., Sonka, A., Anghel, S., Poggiali, G., Belskaya, I., Perna, D., Dotto, E., team, the NEOROCKS
We present new results of the observing program which is a part of the NEOROCKS project aimed to improve knowledge on physical properties of near-Earth Objects (NEOs) for planetary defense. Photometric observations were performed using the 1.2m teles
Externí odkaz:
http://arxiv.org/abs/2302.01165
Autor:
Marsset, M., Brož, M., Vermersch, J., Rambaux, N., Ferrais, M., Viikinkoski, M., Hanuš, J., Jehin, E., Podlewska-Gaca, E., Bartczak, P., Dudzinski, G., Carry, B., Vernazza, P., Szakáts, R., Duffard, R., Jones, A., Molina, D., Santana-Ros, T., Benkhaldoun, Z., Birlan, M., Dumas, C., Fétick, R., Fusco, T., Jorda, L., Marchis, F., Vachier, F., Yang, B.
Cybele asteroids constitute an appealing reservoir of primitive material genetically linked to the outer Solar System, and the physical properties of the largest members can be readily accessed by large telescopes. We took advantage of the bright app
Externí odkaz:
http://arxiv.org/abs/2212.00680
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:
Colas, F., Zanda, B., Bouley, S., Jeanne, S., Malgoyre, A., Birlan, M., Blanpain, C., Gattacceca, J., Jorda, L., Lecubin, J., Marmo, C., Rault, J. L., Vaubaillon, J., Vernazza, P., Yohia, C., Gardiol, D., co-authors, A. Nedelcu plus 300
Publikováno v:
A&A 689, A334 (2024)
Context: Until recently, camera networks designed for monitoring fireballs worldwide were not fully automated, implying that in case of a meteorite fall, the recovery campaign was rarely immediate. This was an important limiting factor as the most fr
Externí odkaz:
http://arxiv.org/abs/2012.00616
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