Zobrazeno 1 - 10
of 55
pro vyhledávání: '"Hodosan, G."'
Publikováno v:
Planetary & Space Science, 204 (2021), 105247
Observations and models suggest that the conditions to develop lightning may be present in cloud-forming extrasolar planetary and brown dwarf atmospheres. Whether lightning on these objects is similar to or very different from what is known from the
Externí odkaz:
http://arxiv.org/abs/2103.10155
Autor:
Hitchcock, J. A., Helling, Ch., Scholz, A., Hodosan, G., Dominik, M., Hundertmark, M., Jørgensen, U. G., Longa-Peña, P., Sajadian, S., Skottfelt, J., Snodgrass, C., Bozza, V., Burgdorf, M. J., Campbell-White, J., Jaimes, Roberto Figuera, Fujii, Y. I., Haikala, L. K., Henning, T., Hinse, T. C., Lowry, S., Mancini, L., Rahvar, S., Rabus, M., Southworth, J., von Essen, C.
We present the results of 14 nights of \textit{I}-band photometric monitoring of the nearby brown dwarf binary, $\epsilon$ Indi Ba,Bb. Observations were acquired over 2 months, and total close to 42 hours of coverage at a typically high cadence of 1.
Externí odkaz:
http://arxiv.org/abs/2005.06906
Autor:
Vinkó, J., Ordasi, A., Szalai, T., Sárneczky, K., Bányai, E., Bíró, I. B., Borkovits, T., Hegedüs, T., Hodosán, G., Kelemen, J., Klagyivik, P., Kriskovics, L., Kun, E., Marion, G. H., Marschalkó, G., Molnár, L., Nagy, A. P., Pál, A., Silverman, J. M., Szakáts, R., Szegedi-Elek, E., Székely, P., Szing, A., Vida, K., Wheeler, J. C.
We present a comparative study of absolute distances to a sample of very nearby, bright Type Ia supernovae (SNe) derived from high cadence, high signal-to-noise, multi-band photometric data. Our sample consists of four SNe: 2012cg, 2012ht, 2013dy and
Externí odkaz:
http://arxiv.org/abs/1804.05815
Autor:
Tanvir, N. R., Levan, A. J., Gonzalez-Fernandez, C., Korobkin, O., Mandel, I., Rosswog, S., Hjorth, J., D'Avanzo, P., Fruchter, A. S., Fryer, C. L., Kangas, T., Milvang-Jensen, B., Rosetti, S., Steeghs, D., Wollaeger, R. T., Cano, Z., Copperwheat, C. M., Covino, S., D'Elia, V., Postigo, A. de Ugarte, Evans, P. A., Even, W. P., Fairhurst, S., Jaimes, R. Figuera, Fontes, C. J., Fujii, Y. I., Fynbo, J. P. U., Gompertz, B. P., Greiner, J., Hodosan, G., Irwin, M. J., Jakobsson, P., Jorgensen, U. G., Kann, D. A., Lyman, J. D., Malesani, D., McMahon, R. G., Melandri, A., O'Brien, P. T., Osborne, J. P., Palazzi, E., Perley, D. A., Pian, E., Piranomonte, S., Rabus, M., Rol, E., Rowlinson, A., Schulze, S., Sutton, P., Thoene, C. C., Ulaczyk, K., Watson, D., Wiersema, K., Wijers, R. A. M. J.
We report the discovery and monitoring of the near-infrared counterpart (AT2017gfo) of a binary neutron-star merger event detected as a gravitational wave source by Advanced LIGO/Virgo (GW170817) and as a short gamma-ray burst by Fermi/GBM and Integr
Externí odkaz:
http://arxiv.org/abs/1710.05455
Autor:
Bozhinova, I., Scholz, A., Costigan, G., Lux, O., Davis, C. J., Ray, T., Boardman, N. F., Hay, K. L., Hewlett, T., Hodosán, G., Morton, B.
RW Aur is a young binary star that experienced a deep dimming in 2010-11 in component A and a second even deeper dimming from summer 2014 to summer 2016. We present new unresolved multi-band photometry during the 2014-16 eclipse, new emission line sp
Externí odkaz:
http://arxiv.org/abs/1609.05667
Autor:
Kóspál, Á., Ábrahám, P., Acosta-Pulido, J. A., Dunham, M. M., García-Álvarez, D., Hogerheijde, M. R., Kun, M., Moór, A., Farkas, A., Hajdu, G., Hodosán, G., Kovács, T., Kriskovics, L., Marton, G., Molnár, L., Pál, A., Sárneczky, K., Sódor, Á., Szakáts, R., Szalai, T., Szegedi-Elek, E., Szing, A., Tóth, I., Vida, K., Vinkó, J.
Publikováno v:
A&A 596, A52 (2016)
HBC 722 (V2493 Cyg) is a young eruptive star in outburst since 2010. It is an FU Orionis-type object with an atypically low outburst luminosity. Because it was well characterized in the pre-outburst phase, HBC 722 is one of the few FUors where we can
Externí odkaz:
http://arxiv.org/abs/1607.05925
Autor:
Hanuš, J., Ďurech, J., Oszkiewicz, D. A., Behrend, R., Carry, B., Delbo', M., Adam, O., Afonina, V., Anquetin, R., Antonini, P., Arnold, L., Audejean, M., Aurard, P., Bachschmidt, M., Badue, B., Barbotin, E., Barroy, P., Baudouin, P., Berard, L., Berger, N., Bernasconi, L., Bosch, J-G., Bouley, S., Bozhinova, I., Brinsfield, J., Brunetto, L., Canaud, G., Caron, J., Carrier, F., Casalnuovo, G., Casulli, S., Cerda, M., Chalamet, L., Charbonnel, S., Chinaglia, B., Cikota, A., Colas, F., Coliac, J-F., Collet, A., Coloma, J., Conjat, M., Conseil, E., Costa, R., Crippa, R., Cristofanelli, M., Damerdji, Y., Debackere, A., Decock, A., Déhais, Q., Déléage, T., Delmelle, S., Demeautis, C., Dróżdż, M., Dubos, G., Dulcamara, T., Dumont, M., Durkee, R., Dymock, R., del Valle, A. Escalante, Esseiva, N., Esseiva, R., Esteban, M., Fauchez, T., Fauerbach, M., Fauvaud, M., Fauvaud, S., Forné, E., Fournel, C., Fradet, D., Garlitz, J., Gerteis, O., Gillier, C., Gillon, M., Giraud, R., Godard, J-P., Goncalves, R., Hamanowa, H., Hay, K., Hellmich, S., Heterier, S., Higgins, D., Hirsch, R., Hodosan, G., Hren, M., Hygate, A., Innocent, N., Jacquinot, H., Jawahar, S., Jehin, E., Jerosimic, L., Klotz, A., Koff, W., Korlevic, P., Kosturkiewicz, E., Krafft, P., Krugly, Y., Kugel, F., Labrevoir, O., Lecacheux, J., Lehký, M., Leroy, A., Lesquerbault, B., Lopez-Gonzales, M. J., Lutz, M., Mallecot, B., Manfroid, J., Manzini, F., Marciniak, A., Martin, A., Modave, B., Montaigut, R., Montier, J., Morelle, E., Morton, B., Mottola, S., Naves, R., Nomen, J., Oey, J., Ogłoza, W., Paiella, M., Pallares, H., Peyrot, A., Pilcher, F., Pirenne, J-F., Piron, P., Polinska, M., Polotto, M., Poncy, R., Previt, J. P., Reignier, F., Renauld, D., Ricci, D., Richard, F., Rinner, C., Risoldi, V., Robilliard, D., Romeuf, D., Rousseau, G., Roy, R., Ruthroff, J., Salom, P. A., Salvador, L., Sanchez, S., Santana-Ros, T., Scholz, A., Séné, G., Skiff, B., Sobkowiak, K., Sogorb, P., Soldán, F., Spiridakis, A., Splanska, E., Sposetti, S., Starkey, D., Stephens, R., Stiepen, A., Stoss, R., Strajnic, J., Teng, J-P., Tumolo, G., Vagnozzi, A., Vanoutryve, B., Vugnon, J. M., Warner, B. D., Waucomont, M., Wertz, O., Winiarski, M., Wolf, M.
Publikováno v:
A&A 586, A108 (2016)
Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation states. This amount already provided a deep insight into physical properties of main-belt asteroids or large collisi
Externí odkaz:
http://arxiv.org/abs/1510.07422
Mineral clouds in substellar atmospheres play a special role as a catalyst for a variety of charge processes. If clouds are charged, the surrounding environment becomes electrically activated, and ensembles of charged grains are electrically discharg
Externí odkaz:
http://arxiv.org/abs/1312.6789
Aims. Hot Jupiters are thought to belong to single-planet systems. Somewhat surprisingly, some hot Jupiters have been reported to exhibit transit timing variations (TTVs). The aim of this paper is to identify the origin of these observations, identif
Externí odkaz:
http://arxiv.org/abs/1207.7229
Autor:
Szabo, Gy. M., Szabo, R., Benko, J. M., Lehmann, H., Mezo, Gy., Simon, A. E., Kovari, Zs., Hodosan, G., Regaly, Zs., Kiss, L. L.
KOI-13.01, a planet-sized companion in an optical double star was announced as one of the 1235 Kepler planet candidates in February 2011. The transit curves show significant distortion that was stable over the ~130 days time-span of the data. Here we
Externí odkaz:
http://arxiv.org/abs/1105.2524