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pro vyhledávání: '"E. Morelle"'
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Akademický článek
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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
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:
E. Morelle-Lauzanne
Publikováno v:
Phytothérapie. 4:234-240
Apres avoir rappele brievement les voies de la lipoperoxydation, cet article developpe l’existence d’une alimentation « oxydative » et d’une alimentation dite « antioxydative ». Ces deux types d’alimentation ont ete mis en evidence par un
Autor:
F. Richard, P. Scheirich, François Colas, E. Morelle, Lawrence A. Molnar, Emmanuel Jehin, M. Bonnardeau, A. Marciniak, M. Birlan, Richard P. Binzel, S. Fauvaud, Stefano Mottola, P. Farissier, M. Fauvaud, A. Leroy, Francesca E. DeMeo, R. Hirsch, C. Gillier, Jean Manfroid, F. Vachier, Marco Delbo, A. Carbognani, Michaël Gillon, Raoul Behrend, Benoit Carry, S. Hellmich, J. Strajnic, K. Sobkowiak, E. Barbotin, A. Matter, Petr Pravec, J. Montier
Publikováno v:
Icarus
Icarus, Elsevier, 2014, 248, pp.516-525. ⟨10.1016/j.icarus.2014.11.002⟩
Icarus, 2014, 248, pp.516-525. ⟨10.1016/j.icarus.2014.11.002⟩
arXiv
Icarus, Elsevier, 2014, 248, pp.516-525. ⟨10.1016/j.icarus.2014.11.002⟩
Icarus, 2014, 248, pp.516-525. ⟨10.1016/j.icarus.2014.11.002⟩
arXiv
In understanding the composition and internal structure of asteroids, their density is perhaps the most diagnostic quantity. We aim here at characterizing the surface composition, mutual orbit, size, mass, and density of the small main-belt binary as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e86b05ed4ee305763b854bd76bbf2835
https://hal.sorbonne-universite.fr/hal-01122881
https://hal.sorbonne-universite.fr/hal-01122881
Autor:
J. Hanuš, J. Ďurech, M. Brož, A. Marciniak, B. D. Warner, F. Pilcher, R. Stephens, R. Behrend, B. Carry, D. Čapek, P. Antonini, M. Audejean, K. Augustesen, E. Barbotin, P. Baudouin, A. Bayol, L. Bernasconi, W. Borczyk, J.-G. Bosch, E. Brochard, L. Brunetto, S. Casulli, A. Cazenave, S. Charbonnel, B. Christophe, F. Colas, J. Coloma, M. Conjat, W. Cooney, H. Correira, V. Cotrez, A. Coupier, R. Crippa, M. Cristofanelli, Ch. Dalmas, C. Danavaro, C. Demeautis, T. Droege, R. Durkee, N. Esseiva, M. Esteban, M. Fagas, G. Farroni, M. Fauvaud, S. Fauvaud, F. Del Freo, L. Garcia, S. Geier, C. Godon, K. Grangeon, H. Hamanowa, N. Heck, S. Hellmich, D. Higgins, R. Hirsch, M. Husarik, T. Itkonen, O. Jade, K. Kamiński, P. Kankiewicz, A. Klotz, R. A. Koff, A. Kryszczyńska, T. Kwiatkowski, A. Laffont, A. Leroy, J. Lecacheux, Y. Leonie, C. Leyrat, F. Manzini, A. Martin, G. Masi, D. Matter, J. Michałowski, M. J. Michałowski, T. Michałowski, J. Michelet, R. Michelsen, E. Morelle, S. Mottola, R. Naves, J. Nomen, J. Oey, W. Ogłoza, A. Oksanen, D. Oszkiewicz, P. Pääkkönen, M. Paiella, H. Pallares, J. Paulo, M. Pavic, B. Payet, M. Polińska, D. Polishook, R. Poncy, Y. Revaz, C. Rinner, M. Rocca, A. Roche, D. Romeuf, R. Roy, H. Saguin, P. A. Salom, S. Sanchez, G. Santacana, T. Santana-Ros, J.-P. Sareyan, K. Sobkowiak, S. Sposetti, D. Starkey, R. Stoss, J. Strajnic, J.-P. Teng, B. Trégon, A. Vagnozzi, F. P. Velichko, N. Waelchli, K. Wagrez, H. Wücher
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2013, 551 (A67), 16 p. ⟨10.1051/0004-6361/201220701⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2013, 551 (A67), 16 p. ⟨10.1051/0004-6361/201220701⟩
Astronomy and Astrophysics-A&A, 2013, 551 (A67), 16 p. ⟨10.1051/0004-6361/201220701⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2013, 551 (A67), 16 p. ⟨10.1051/0004-6361/201220701⟩
The larger number of models of asteroid shapes and their rotational states derived by the lightcurve inversion give us better insight into both the nature of individual objects and the whole asteroid population. With a larger statistical sample we ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c4f9941a036a9dd815e01cce509f1298
https://hal.science/hal-00794404
https://hal.science/hal-00794404
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
Akademický článek
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