Zobrazeno 1 - 10 of 53 pro vyhledávání: '"F. Marchis"'
2
The equilibrium shape of (65) Cybele: primordial or relic of a large impact?
Autor: M. Marsset, M. Brož, J. Vermersch, N. Rambaux, M. Ferrais, M. Viikinkoski, J. Hanuš, E. Jehin, E. Podlewska-Gaca, P. Bartczak, G. Dudziński, B. Carry, P. Vernazza, R. Szakáts, R. Duffard, A. Jones, D. Molina, T. Santana-Ros, Z. Benkhaldoun, M. Birlan, C. Dumas, R. Fétick, T. Fusco, L. Jorda, F. Marchis, F. Vachier, B. Yang
Publikováno v: Astronomy & Astrophysics. 670:A52
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4f7f1d7e36c4962622a3b609b3df609b
https://doi.org/10.1051/0004-6361/202243859
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3
Observed tidal evolution of Kleopatra's outer satellite
Autor: M. Walterova, Laurent Jorda, F. Marchis, M. Broz, Raoul Behrend, Josef Hanus, David Vokrouhlicky, J. Durech, F. Vachier, Benoit Carry, Pierre Vernazza
Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 657, ⟨10.1051/0004-6361/202142055⟩
The orbit of the outer satellite Alexhelios of (216) Kleopatra is already constrained by adaptive-optics astrometry, obtained with the VLT/SPHERE instrument. However, there is also a preceding occultation event in 1980 attributed to this satellite. H
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92982d194e1a02d262e9a5fd24260d73
http://arxiv.org/abs/2110.12702
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4
VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis
Autor: J. Krajewski, P. Aurard, Philippe Lamy, Vishnu Reddy, Laurent Jorda, D. Molina, Josef Hanus, Josef Ďurech, P. Michel, F. Vachier, Nicolas Rambaux, J. Oey, Grzegorz Dudziński, P. Bartczak, A. Leroy, Michael Marsset, L. Dalmon, P. Beck, H. Le Coroller, Hiroko Hamanowa, Maëlle Neveu, Christophe Dumas, Hiromi Hamanowa, A. G. Sanchez, Zouhair Benkhaldoun, N. Payre, E. Podlewska-Gaca, Fabrice Cipriani, Raoul Behrend, Paolo Tanga, Aled Jones, Julie Castillo-Rogez, Miroslav Brož, P. Antonini, Tadeusz Michalowski, F. Livet, O. Labrevoir, J. M. Bosch, Emmanuel Jehin, Arthur Vigan, S. Fauvaud, A. Chapman, Marin Ferrais, Jérôme Berthier, Alexis Drouard, Mirel Birlan, J. Grice, R. Montaigut, J. His, L. Socha, Romain Fétick, Olivier Witasse, Pierre Vernazza, Thierry Fusco, Benoit Carry, F. Marchis, Doeon Kim, Toni Santana-Ros, Mikko Kaasalainen, Matti Viikinkoski, P. Sabin, M. Audejean, A. Marciniak, Myung-Jin Kim, Bin Yang, Agnieszka Kryszczyńska, François Colas
Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A56. ⟨10.1051/0004-6361/202141781⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A, 2021, 654, pp.A56. ⟨10.1051/0004-6361/202141781⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Vernazza, P., et al.
Until recently, the 3D shape, and therefore density (when combining the volume estimate with available mass estimates), and surface topography of the vast majority of the largest (D ≥ 100 km) main-belt asteroids have remai
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a582d603789efa8c1fec089600157a07
https://hal.archives-ouvertes.fr/hal-03375585/document
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5
The Future of Planetary Defense in the Era of Advanced Surveys
Autor: R. T. Daly, Timothy D. Swindle, Sean E. Marshall, Marco Delbo, A. Wong, T. Grav, Judy Pipher, Sarah Greenstreet, Alan Stern, Amy Mainzer, D. C. Hickson, Kynan H.G. Hughson, Joseph Lazio, Daniel T. Britt, B. Betts, Rosaly M. C. Lopes, Michele T. Bannister, Edgard G. Rivera-Valentín, Mario Juric, Peter Eisenhardt, Sean Carey, Walter M. Harris, James F. Bell, Joseph Masiero, Robert S. McMillan, Maria Gritsevich, Daniel J. Scheeres, Devanshu Jha, M. Bruckner, Alan W. Harris, D. Takir, C. A. Schambeau, F. Marchis, Michael C. Nolan, Flaviane Venditti, Betul Kacar, T. Okada, Yan Fernandez, P. Michel, Patrick A. Taylor, C. McMurtry, Ronald A. Fevig, William F. Bottke, P. Abell, Jennifer E.C. Scully, J. Barnes, Cristina A. Thomas, Maitrayee Bose, D. Cotto-Figueroa, J. Chesley, Anne Virkki, P. W. Chodas, Timothy Spahr, D. Mathias, Brent W. Barbee, Lance A. M. Benner, Michael W. Busch, Shantanu P. Naidu, Carol A. Raymond, Heidi B. Hammel, M. Brozovic, Željko Ivezić, Lynne Jones, E. Christensen, M. Telus, Julie Castillo-Rogez, Dante S. Lauretta, S. Sonnett, Andrew S. Rivkin, Edward L. Wright, J. Dotson
Publikováno v: Bulletin of the AAS
Bulletin of the AAS, American Astronomical Society, 2021, 53 (4), ⟨10.3847/25c2cfeb.ba7af878⟩
International audience
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::82e3d5031af92d1066f11febdd1f4a8b
https://hal-insu.archives-ouvertes.fr/insu-03413444/file/PlanetaryDefense_DecadalSurvey_BAAS53.pdf
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6
Physical characterization of double asteroid (617) Patroclus from 2007/2012 mutual events observations
Autor: F. Colas, Florent Deleflie, Felipe Braga-Ribas, J. Normand, Hiromi Hamanowa, Alain Klotz, Pascal Descamps, P. Vingerhoets, J. A. Farrell, L. Maquet, K. Archer, G. Dubos, Vishnu Reddy, T. Pauwels, Frédéric Vachier, A. Peyrot, Joe Pollock, F. Marchis, A. Leroy, Pedro V. Sada, Jérôme Berthier, Sylvain Bouley, J.-P. Teng-Chuen-Yu
Publikováno v: Icarus
Icarus, Elsevier, 2020, ⟨10.1016/j.icarus.2020.113990⟩
Icarus, 2020, ⟨10.1016/j.icarus.2020.113990⟩
HAL
International audience; We publish a set of 16 light curves of mutual events inside the synchronous system of the Jupiter Trojan (617) Patroclus. Patroclus is th only binary system of the six target asteroids of the forthcoming NASA Discovery-class m
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c74b5d2ba0b746c13726ed44931ba404
https://hal.archives-ouvertes.fr/hal-03023849
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7
Volume uncertainty of (7) Iris shape models from disc-resolved images
Autor: Laurent Jorda, P. Michel, Miroslav Brož, Michael Marsset, P. Bartczak, H. Le Coroller, Jérôme Berthier, Matti Viikinkoski, Paolo Tanga, Marin Ferrais, Benoit Carry, Arthur Vigan, Bin Yang, Pierre Vernazza, P. L. Lamy, Christophe Dumas, Tadeusz Michalowski, Toni Santana-Ros, Alexis Drouard, Romain Fétick, Grzegorz Dudziński, Julie Castillo-Rogez, M. Birlan, F. Vachier, S. Benseguane, Thierry Fusco, Agnieszka Kryszczyńska, E. Podlewska-Gaca, Fabrice Cipriani, Olivier Witasse, F. Marchis, Josef Hanus, Nicolas Rambaux, Emmanuel Jehin, A. Marciniak, François Colas
Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 499 (3), pp.4545-4560. ⟨10.1093/mnras/staa3153⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (3), pp.4545-4560. ⟨10.1093/mnras/staa3153⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
High angular resolution disc-resolved images of (7) Iris collected by VLT/SPHERE instrument are allowed for the detailed shape modelling of this large asteroid revealing its surface features. If (7) Iris did not suffer any events catastrophic enough
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3c9a707581bce97a50c0a2abd7c23eb
https://hdl.handle.net/10045/111480
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8
Asteroid (16) Psyche’s primordial shape: A possible Jacobi ellipsoid
Autor: P. Bartczak, A. Marciniak, E. Podlewska-Gaca, Bin Yang, Fabrice Cipriani, Miroslav Brož, Arthur Vigan, Tadeusz Michalowski, Julie Castillo-Rogez, F. Vachier, Patrick Michel, Benoit Carry, Olivier Witasse, François Colas, Pierre Vernazza, F. Marchis, Emmanuel Jehin, P. Lamy, Josef Hanus, Matti Viikinkoski, Nicolas Rambaux, Romain Fétick, Alexis Drouard, Toni Santana-Ros, H. Le Coroller, M. Birlan, Mikko Kaasalainen, Agnieszka Kryszczyńska, Laurent Jorda, Josef Ďurech, Michael Marsset, Grzegorz Dudziński, Paolo Tanga, Marin Ferrais, Thierry Fusco, Christophe Dumas, Jérôme Berthier
Publikováno v: RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 638, pp.L15. ⟨10.1051/0004-6361/202038100⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.L15. ⟨10.1051/0004-6361/202038100⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Context. Asteroid (16) Psyche is the largest M-type asteroid in the main belt and the target of the NASA Psyche mission. It is also the only asteroid of this size (D> 200 km) known to be metal rich. Although various hypotheses have been proposed to e
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83733fbb3753743301e56f53ea990f2e
http://hdl.handle.net/10045/108214
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10
A basin-free spherical shape as an outcome of a giant impact on asteroid Hygiea
Autor: J. Grice, Mikko Kaasalainen, F. Colas, A. Chapman, Tadeusz Michalowski, Arthur Vigan, Josef Hanus, Julie Castillo-Rogez, Róbert Szakáts, Marin Ferrais, Przemyslaw Bartczak, Benoit Carry, Miroslav Brož, Laurent Jorda, Nicolas Rambaux, Matti Viikinkoski, Grzegorz Dudziński, P. Michel, Agnieszka Kryszczyńska, Rene Duffard, Michaël Gillon, Michael Marsset, Jérôme Berthier, J. Durech, Bin Yang, Mirel Birlan, Christophe Dumas, R. Hirsch, Francesca E. DeMeo, F. Vachier, P. Lamy, Toni Santana-Ros, Thierry Fusco, Zouhair Benkhaldoun, E. Podlewska-Gaca, Fabrice Cipriani, P. Ševeček, H. Le Coroller, Olivier Witasse, A. Marciniak, F. Marchis, Emmanuel Jehin, J. L. Maestre, Alexis Drouard, Romain Fétick, Pierre Vernazza, Paolo Tanga
Publikováno v: Nature Astronomy
Nature Astronomy, Nature Publishing Group, 2019, 4, pp.136-141. ⟨10.1038/s41550-019-0915-8⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Nature Astronomy, 2019, 4, pp.136-141. ⟨10.1038/s41550-019-0915-8⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
(10) Hygiea is the fourth largest main belt asteroid and the only known asteroid whose surface composition appears similar to that of the dwarf planet (1) Ceres1,2, suggesting a similar origin for these two objects. Hygiea suffered a giant impact mor
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d29caac3c1f8e64c76e67cb246404591
https://hal.archives-ouvertes.fr/hal-02346869/file/PV_Final.pdf
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