Zobrazeno 1 - 10
of 46
pro vyhledávání: '"Slyusarev, I."'
Autor:
Ďurech, J., Vokrouhlický, D., Pravec, P., Krugly, Yu., Polishook, D., Hanuš, J., Marchis, F., Rożek, A., Snodgrass, C., Alegre, L., Donchev, Z., Ehgamberdiev, Sh. A., Fatka, P., Gaftonyuk, N. M., Galád, A., Hornoch, K., Inasaridze, R. Ya., Khalouei, E., Kučáková, H., Kušnirák, P., Oey, J., Pray, D. P., Sergeev, A., Slyusarev, I.
The rotation state of small asteroids is affected in the long term by perturbing torques of gravitational and radiative origin (the YORP effect). Direct observational evidence of the YORP effect is the primary goal of our work. We carried out photome
Externí odkaz:
http://arxiv.org/abs/2312.05157
Autor:
Rommel, F. L., Braga-Ribas, F., Ortiz, J. L., Sicardy, B., Santos-Sanz, P., Desmars, J., Camargo, J. I. B., Vieira-Martins, R., Assafin, M., Morgado, B. E., Boufleur, R. C., Benedetti-Rossi, G., Gomes-Júnior, A. R., Fernández-Valenzuela, E., Holler, B. J., Souami, D., Duffard, R., Margoti, G., Vara-Lubiano, M., Lecacheux, J., Plouvier, J. L., Morales, N., Maury, A., Fabrega, J., Ceravolo, P., Jehin, E., Albanese, D., Mariey, H., Cikota, S., Ruždjak, D., Cikota, A., Szakáts, R., Aissa, D. Baba, Gringahcene, Z., Kashuba, V., Koshkin, N., Zhukov, V., Fişek, S., Çakır, O., Özer, S., Schnabel, C., Schnabel, M., Signoret, F., Morrone, L., Santana-Ros, T., Pereira, C. L., Emilio, M., Burdanov, A. Y., de Wit, J., Barkaoui, K., Gillon, M., Leto, G., Frasca, A., Catanzaro, G., Sanchez, R. Zanmar, Tagliaferri, U., Di Sora, M., Isopi, G., Krugly, Y., Slyusarev, I., Chiorny, V., Mikuž, H., Bacci, P., Maestripieri, M., Grazia, M. D., de la Cueva, I., Yuste-Moreno, M., Ciabattari, F., Kozhukhov, O. M., Serra-Ricart, M., Alarcon, M. R., Licandro, J., Masi, G., Bacci, R., Bosch, J. M., Behem, R., Prost, J. -P., Renner, S., Conjat, M., Bachini, M., Succi, G., Stoian, L., Juravle, A., Carosati, D., Gowe, B., Carrillo, J., Zheleznyak, A. P., Montigiani, N., Foster, C. R., Mannucci, M., Ruocco, N., Cuevas, F., Di Marcantonio, P., Coretti, I., Iafrate, G., Baldini, V., Collins, M., Pál, A., Csák, B., Fernández-Garcia, E., Castro-Tirado, A. J., Hudin, L., Madiedo, J. M., Anghel, R. M., Calvo-Fernández, J. F., Valvasori, A., Guido, E., Gherase, R. M., Kamoun, S., Fafet, R., Sánchez-González, M., Curelaru, L., Vîntdevară, C. D., Danescu, C. A., Gout, J. -F., Schmitz, C. J., Sota, A., Belskaya, I., Rodríguez-Marco, M., Kilic, Y., Frappa, E., Klotz, A., Lavayssière, M., Oliveira, J. Marques, Popescu, M., Mammana, L. A., Fernández-Lajús, E., Schmidt, M., Hopp, U., Komžík, R., Pribulla, T., Tomko, D., Husárik, M., Erece, O., Eryilmaz, S., Buzzi, L., Gährken, B., Nardiello, D., Hornoch, K., Sonbas, E., Er, H., Burwitz, V., Sybilski, P. Waldemar, Bykowski, W., Müller, T. G., Ogloza, W., Gonçalves, R., Ferreira, J. F., Ferreira, M., Bento, M., Meister, S., Bagiran, M. N., Tekeş, M., Marciniak, A., Moravec, Z., Delinčák, P., Gianni, G., Casalnuovo, G. B., Boutet, M., Sanchez, J., Klemt, B., Wuensche, N., Burzynski, W., Borkowski, M., Serrau, M., Dangl, G., Klös, O., Weber, C., Urbaník, M., Rousselot, L., Kubánek, J., André, P., Colazo, C., Spagnotto, J., Sickafoose, A. A., Hueso, R., Sánchez-Lavega, A., Fisher, R. S., Rengstorf, A. W., Perelló, C., Dascalu, M., Altan, M., Gazeas, K., de Santana, T., Sfair, R., Winter, O. C., Kalkan, S., Canales-Moreno, O., Trigo-Rodríguez, J. M., Tsamis, V., Tigani, K., Sioulas, N., Lekkas, G., Bertesteanu, D. N., Dumitrescu, V., Wilberger, A. J., Barnes, J. W., Fieber-Beyer, S. K., Swaney, R. L., Fuentes, C., Mendez, R. A., Dumitru, B. D., Flynn, R. L., Wake, D. A.
Publikováno v:
A&A 678, A167 (2023)
This work aims at constraining the size, shape, and geometric albedo of the dwarf planet candidate 2002 MS4 through the analysis of nine stellar occultation events. Using multichord detection, we also studied the object's topography by analyzing the
Externí odkaz:
http://arxiv.org/abs/2308.08062
Autor:
Shevchenko1, V. G., Inasaridze, R. Ya., Krugly, Yu. N., Ayvazian, V. V., Kapanadze, G. V., Datashvili, G., Slyusarev, I. G., Chiorny, V. G., Molotov, I. E.
In frame of an implementation of the cooperative program studying of asteroids between the Kharadze Abastumani Astrophysical Observatory and the Astronomical Institute of V.N. Karazin Kharkiv National University the observations for five main-belt as
Externí odkaz:
http://arxiv.org/abs/2201.00347
Autor:
Shevchenko, V., Mikhalchenko, O., Belskaya, I., Slyusarev, I., Chiorny, V., Krugly, Yu., Hromakina, T., Dovgopol, A., Kiselev, N., Rublevsky, A., Antonyuk, K., Novichonok, A., Kusakin, A., Reva, I., Inasaridze, R., Ayvazian, V., Kapanadze, G., Molotov, I., Oszkiewicz, D., Kwiatkowski, T.
We present new photometric observations for twelve asteroids ((122) Gerda, (152) Atala, (260) Huberta, (665) Sabine, (692) Hippodamia, (723) Hammonia, (745) Mauritia, (768) Struveana, (863) Benkoela, (1113) Katja, (1175) Margo, (2057) Rosemary) from
Externí odkaz:
http://arxiv.org/abs/2105.09763
Autor:
Hromakina, T., Belskaya, I., Krugly, Yu., Rumyantsev, V., Golubov, O., Kyrylenko, I., Ivanova, O., Velichko, S., Izvekova, I., Sergeyev, A., Slyusarev, I., Molotov, I.
Publikováno v:
A&A 647, A71 (2021)
Less than one percent of the discovered small solar system objects have highly inclined orbits ($i>60^{\circ}$), and revolve around the Sun on near-polar or retrograde orbits. The origin and evolutionary history of these objects are not yet clear. In
Externí odkaz:
http://arxiv.org/abs/2101.04541
Autor:
Pravec, P., Fatka, P., Vokrouhlický, D., Scheirich, P., Ďurech, J., Scheeres, D. J., Kušnirák, P., Hornoch, K., Galád, A., Pray, D. P., Krugly, Yu. N., Burkhonov, O., Ehgamberdiev, Sh. A., Pollock, J., Moskovitz, N., Ortiz, J. L., Morales, N., Husárik, M., Inasaridze, R. Ya., Oey, J., Polishook, D., Hanuš, J., Kučáková, H., Vraštil, J., Világi, J., Gajdoš, Š., Kornoš, L., Vereš, P., Gaftonyuk, N. M., Hromakina, T., Sergeyev, A. V., Slyusarev, I. G., Ayvazian, V. R., Cooney, W. R., Gross, J., Terrell, D., Colas, F., Vachier, F., Slivan, S., Skiff, B., Marchis, F., Ergashev, K. E., Aznar, D. -H. Kim A., Serra-Ricart, M., Behrend, R., Roy, R., Manzini, F., Molotov, I. E.
We studied 93 asteroid pairs. We estimated times elapsed since separation of pair members that are between 7*10^3 and a few 10^6 yr. We derived the rotation periods for all the primaries and a sample of secondaries. We derived the absolute magnitude
Externí odkaz:
http://arxiv.org/abs/1901.05492
Akademický článek
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Autor:
Scheirich, P., Pravec, P., Jacobson, S. A., Ďurech, J., Kušnirák, P., Hornoch, K., Mottola, S., Mommert, M., Hellmich, S., Pray, D., Polishook, D., Krugly, Yu. N., Inasaridze, R. Ya., Kvaratskhelia, O. I., Ayvazian, V., Slyusarev, I., Pittichová, J., Jehin, E., Manfroid, J., Gillon, M., Galád, A., Pollock, J., Licandro, J., Alí-Lagoa, V., Brinsfield, J., Molotov, I. E.
Publikováno v:
Icarus 245 (2015) 56-63
Using our photometric observations taken between 1996 and 2013 and other published data, we derived properties of the binary near-Earth asteroid (175706) 1996 FG3 including new measurements constraining evolution of the mutual orbit with potential co
Externí odkaz:
http://arxiv.org/abs/1406.4677
Autor:
Durech, J., Vokrouhlicky, D., Baransky, A. R., Breiter, S., Burkhonov, O. A., Cooney, W., Fuller, V., Gaftonyuk, N. M., Gross, J., Inasaridze, R. Ya., Kaasalainen, M., Krugly, Yu. N., Kvaratshelia, O. I., Litvinenko, E. A., Macomber, B., Marchis, F., Molotov, I. E., Oey, J., Polishook, D., Pollock, J., Pravec, P., Sarneczky, K., Shevchenko, V. G., Slyusarev, I., Stephens, R., Szabo, Gy., Terrell, D., Vachier, F., Vanderplate, Z., Viikinkoski, M., Warner, B. D.
The spin state of small asteroids can change on a long timescale by the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect, the net torque that arises from anisotropically scattered sunlight and proper thermal radiation from an irregularly-shaped as
Externí odkaz:
http://arxiv.org/abs/1210.2219
Autor:
Pandey, S. B., Castro-Tirado, A. J., Jelínek, M., Kamble, Atish P., Gorosabel, J., Postigo, A. de Ugarte, Prins, S., Oreiro, R., Chantry, V., Trushkin, S., Bremer, M., Winters, J. M., Pozanenko, A., Krugly, Yu., Slyusarev, I., Kornienko, G., Erofeeva, A., Misra, K., Ramprakash, A. N., Mohan, V., Bhattacharya, D., Volnova, A., Plá, J., Ibrahimov, M., Im, M., Volvach, A., Wijers, R. A. M. J.
We present observations of the afterglow of GRB 080319B at optical, mm and radio frequencies from a few hours to 67 days after the burst. Present observations along with other published multi-wavelength data have been used to study the light-curves a
Externí odkaz:
http://arxiv.org/abs/0904.1797