Zobrazeno 1 - 10
of 43
pro vyhledávání: '"M. Lehký"'
Autor:
Hana Kučáková, M. Lehký, K. Hoňková, Martin Mašek, L. Smelcer, P. Zasche, K. Hornoch, Marek Wolf, Jakub Juryšek
Publikováno v:
Contributions of the Astronomical Observatory Skalnaté Pleso. 50
Autor:
Josef Ďurech, Hong-Kyu Moon, Hee-Jae Lee, Murat Kaplan, Adrian Galad, Anna Marciniak, Jozef Vilagi, Rene Duffard, Štefan Gajdoš, Young-Jun Choi, D. P. Pray, M. Lehký, Myung-Jin Kim, Orhan Erece, Chun-Hwey Kim
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Context. The study of non-principal axis (NPA) rotators can provide important clues to the evolution of the spin state of asteroids. However, very few studies to date have focused on NPA-rotating main belt asteroids (MBAs). One MBA known to be in an
Autor:
K. Hoňková, Hana Kučáková, Jakub Juryšek, L. Kotková, A. Paschke, Martin Mašek, Petr Cagas, R. Uhlař, Marek Wolf, Danielle Bewsher, Martin Jelínek, Petr Zasche, Glenn J. White, M. Lehký, M. Tylšar
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The full Table 1 is only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/619/A85
We present an analysis of the apsidal motion and light curve parameters of 54 neve
We present an analysis of the apsidal motion and light curve parameters of 54 neve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c38d4dc37abfc230910d1ec6f06e181
http://hdl.handle.net/10261/209201
http://hdl.handle.net/10261/209201
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:
N. Gaftonyuk, Julian Oey, Peter Kusnirak, Josef Hanus, O. Kvaratskhelia, Igor Molotov, Roger Groom, Vasilij G. Chiorny, Hana Kučáková, Vasilij G. Shevchenko, Kamil Hornoch, J. Vrastil, Brian D. Warner, Yu. N. Krugly, Josef Ďurech, R. Inasaridze, P. Pravec, Adrian Galad, David Vokrouhlický, M. Lehký, P. Fatka, Davide Farnocchia, V. R. Ayvazian, Joe Pollock, G. Masi
Context. The rotation states of small asteroids are affected by a net torque arising from an anisotropic sunlight reflection and thermal radiation from the asteroids’ surfaces. On long timescales, this so-called YORP effect can change asteroid spin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83b6cda57f1c72ba79e50e70c2185829
http://arxiv.org/abs/1711.05987
http://arxiv.org/abs/1711.05987
Autor:
M. Bělík, Martin Mašek, K. Hoňková, Marek Wolf, Ladislav Šmelcer, M. Tylšar, Hana Kučáková, M. Lehký, J. Vrastil, Kamil Hornoch, Rudolf Novak, L. Červinka, Petr Zasche
Publikováno v:
Astronomy & Astrophysics. 620:A72
We present the next results of our long-term observational project to analyze the variations in the orbital periods of low-mass eclipsing binaries. About 70 new precise mid-eclipse times recorded with a CCD were obtained for two eclipsing binaries wi
Akademický článek
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Publikováno v:
New Astronomy. 16:402-404
Several new precise times of eclipses were measured for eclipsing binary CG Aur as a part of our long-term observational project for studying eclipsing binaries with an eccentric orbit. Based on a current O − C diagram, we found for the first time
Autor:
Miloslav Zejda, Hana Kučáková, M. Lehký, Ladislav Šmelcer, Petr Zasche, P. Svoboda, Marek Wolf
Aims. As part of the long-term Ondrejov and Ostrava observational projects, we aim to measure the precise times of minimum light for eccentric eclipsing binaries, needed for accurate determination of apsidal motion. Over fifty new times of minimum li
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ed05c9094e0c2c595d605a7cb6e7e52
http://hdl.handle.net/10084/123968
http://hdl.handle.net/10084/123968
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