Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Hiromi Hamanowa"'
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
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
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
https://hal.archives-ouvertes.fr/hal-03375585/document
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
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
https://hal.archives-ouvertes.fr/hal-03023849
Autor:
Josef Hanus, Luc Arnold, Maria J. Esteban, E. Morelle, H. Gully, P. Antonini, Peter Kusnirak, Silvano Casulli, Marco Delbo, F. Manzini, P. Pravec, H. Cibulková, Bryce Bolin, Victor Ali-Lagoa, J. Michelet, Josef Ďurech, M. Lehký, H. de Groot, R. Dymock, L. Bernasconi, M. Bachschmidt, M. Audejean, Julian Oey, P. A. Salom, Robert Jedicke, N. Esseiva, Brian D. Warner, L. Brunetto, Raoul Behrend, F. Marchis, Rupak Roy, Frederick Pilcher, Hiroko Hamanowa, F. Reignier, P. Krafft, Hiromi Hamanowa, O. Gerteis
Publikováno v:
Icarus
Icarus, Elsevier, 2018, 299, pp.84-96. ⟨10.1016/j.icarus.2017.07.007⟩
Icarus, Elsevier, 2018, 299, pp.84-96. ⟨10.1016/j.icarus.2017.07.007⟩
Eos family was created during a catastrophic impact about 1.3 Gyr ago. Rotation states of individual family members contain information about the history of the whole population. We aim to increase the number of asteroid shape models and rotation sta
Publikováno v:
International Journal of Astronomy and Astrophysics. :193-207
Some evidences of possible duplicities of five asteroids are presented. A satellite of (279) Thule was convincingly detected by a stellar occultation on 2008 April 3 by Thule and also from follow-up light curve observations. The orbital period of the
Publikováno v:
International Journal of Astronomy and Astrophysics. :91-118
A 3-D shape model of the sixth largest of the main belt asteroids, (704) Interamnia, is presented. The model is reproduced from its two stellar occultation observations and six lightcurves between 1969 and 2011. The first stellar occultation was the
Autor:
Jean Manfroid, Marco Delbo, C. Vera Hernández, J. Lecacheux, Raoul Behrend, E. Frappa, Paolo Tanga, Julio Camargo, M. Audejean, Lucie Maquet, M. Conjat, Maxime Devogele, G. Dubos, M. Todd, Magdalena Polińska, N. Cornero, R. Roy, M. Cedrés Reyes, D. Coward, Marcelo Assafin, V. Alí Lagoa, A. Klotz, Hiromi Hamanowa, E. Morelle, F. Manzini, R. Crippa, Emmanuel Jehin, Frédéric Vachier, A. Matter, A. H. Andrei, A. Leroy, E. de Ferra Fantin, Albino Carbognani, P. Wiggins, Stefano Mottola, François Colas, Agnieszka Kryszczyńska, Michaël Gillon, Benoit Carry, Josef Hanus
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 448 (4), pp.3382-3390. ⟨10.1093/mnras/stv229⟩
Monthly Notices of the Royal Astronomical Society, 2015, 448 (4), pp.3382-3390. ⟨10.1093/mnras/stv229⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 448 (4), pp.3382-3390. ⟨10.1093/mnras/stv229⟩
Monthly Notices of the Royal Astronomical Society, 2015, 448 (4), pp.3382-3390. ⟨10.1093/mnras/stv229⟩
Asteroid (234) Barbara is the prototype of a category of asteroids that has been shown to be extremely rich in refractory inclusions, the oldest material ever found in the Solar System. It exhibits several peculiar features, most notably its polarime
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b61165d2d5178afbeb91eba76303dd2d
https://hal.archives-ouvertes.fr/hal-02483528
https://hal.archives-ouvertes.fr/hal-02483528
Autor:
J. Hanuš, J. Ďurech, D. A. Oszkiewicz, R. Behrend, B. Carry, M. Delbo, O. Adam, V. Afonina, R. Anquetin, P. Antonini, L. Arnold, M. Audejean, P. Aurard, M. Bachschmidt, B. Baduel, E. Barbotin, P. Barroy, P. Baudouin, L. Berard, N. Berger, L. Bernasconi, J-G. Bosch, S. Bouley, I. Bozhinova, J. Brinsfield, L. Brunetto, G. Canaud, J. Caron, F. Carrier, G. Casalnuovo, S. Casulli, M. Cerda, L. Chalamet, S. Charbonnel, B. Chinaglia, A. Cikota, F. Colas, J.-F. Coliac, A. Collet, J. Coloma, M. Conjat, E. Conseil, R. Costa, R. Crippa, M. Cristofanelli, Y. Damerdji, A. Debackère, A. Decock, Q. Déhais, T. Déléage, S. Delmelle, C. Demeautis, M. Dróżdż, G. Dubos, T. Dulcamara, M. Dumont, R. Durkee, R. Dymock, A. Escalante del Valle, N. Esseiva, R. Esseiva, M. Esteban, T. Fauchez, M. Fauerbach, M. Fauvaud, S. Fauvaud, E. Forné, C. Fournel, D. Fradet, J. Garlitz, O. Gerteis, C. Gillier, M. Gillon, R. Giraud, J.-P. Godard, R. Goncalves, Hiroko Hamanowa, Hiromi Hamanowa, K. Hay, S. Hellmich, S. Heterier, D. Higgins, R. Hirsch, G. Hodosan, M. Hren, A. Hygate, N. Innocent, H. Jacquinot, S. Jawahar, E. Jehin, L. Jerosimic, A. Klotz, W. Koff, P. Korlevic, E. Kosturkiewicz, P. Krafft, Y. Krugly, F. Kugel, O. Labrevoir, J. Lecacheux, M. Lehký, A. Leroy, B. Lesquerbault, M. J. Lopez-Gonzales, M. Lutz, B. Mallecot, J. Manfroid, F. Manzini, A. Marciniak, A. Martin, B. Modave, R. Montaigut, J. Montier, E. Morelle, B. Morton, S. Mottola, R. Naves, J. Nomen, J. Oey, W. Ogłoza, M. Paiella, H. Pallares, A. Peyrot, F. Pilcher, J.-F. Pirenne, P. Piron, M. Polińska, M. Polotto, R. Poncy, J. P. Previt, F. Reignier, D. Renauld, D. Ricci, F. Richard, C. Rinner, V. Risoldi, D. Robilliard, D. Romeuf, G. Rousseau, R. Roy, J. Ruthroff, P. A. Salom, L. Salvador, S. Sanchez, T. Santana-Ros, A. Scholz, G. Séné, B. Skiff, K. Sobkowiak, P. Sogorb, F. Soldán, A. Spiridakis, E. Splanska, S. Sposetti, D. Starkey, R. Stephens, A. Stiepen, R. Stoss, J. Strajnic, J.-P. Teng, G. Tumolo, A. Vagnozzi, B. Vanoutryve, J. M. Vugnon, B. D. Warner, M. Waucomont, O. Wertz, M. Winiarski, M. Wolf
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2016, 586, pp.A108. ⟨10.1051/0004-6361/201527441⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 586, pp.A108. ⟨10.1051/0004-6361/201527441⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2016, 586, pp.A108. ⟨10.1051/0004-6361/201527441⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 586, pp.A108. ⟨10.1051/0004-6361/201527441⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Context. Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation states. These efforts already provided deep insight into physical properties of main-belt asteroids or larg
Autor:
Eloy Sira, Ignacio Ferrin, Haibin Zhao, Hiromi Hamanowa, Hiroko Hamanowa, Richard Miles, Albert Sánchez, Jesús Hernández
(1) We find that comet 107P/WH was active in 1949, 1979, 1992, 2005, and 2009. (2) Its age can be measured. We find T-AGE=4700 comet years, WB-AGE=7800 cy. (3) This is a methuselah comet very near to its dormancy phase, being temporarily rejuvenated
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::245d166933d6c68f45e434749ecc0b4c