Zobrazeno 1 - 10
of 64
pro vyhledávání: '"Charbonnel, S."'
Autor:
Merc, J., Gális, R., Velez, P., Charbonnel, S., Garde, O., Dû, P. Le, Mulato, L., Petit, T., Bohlsen, T., Curry, S., Love, T., Barker, H.
V618 Sgr was previously classified as an R CrB-type variable and later as a possible symbiotic star. Our study aims to analyse the nature of this target, which is currently undergoing significant brightening in properties similar to those of known sy
Externí odkaz:
http://arxiv.org/abs/2305.03537
Autor:
Hanuš, J., Vernazza, P., Viikinkoski, M., Ferrais, M., Rambaux, N., Podlewska-Gaca, E., Drouard, A., Jorda, L., Jehin, E., Carry, B., Marsset, M., Marchis, F., Warner, B., Behrend, R., Asenjo, V., Berger, N., Bronikowska, M., Brothers, T., Charbonnel, S., Colazo, C., Coliac, J-F., Duffard, R., Jones, A., Leroy, A., Marciniak, A., Melia, R., Molina, D., Nadolny, J., Person, M., Pejcha, O., Riemis, H., Shappee, B., Sobkowiak, K., Soldán, F., Suys, D., Szakats, R., Vantomme, J., Birlan, M., Berthier, J., Bartczak, P., Dumas, C., Dudziński, G., Ďurech, J., Castillo-Rogez, J., Cipriani, F., Fetick, R., Fusco, T., Grice, J., Kaasalainen, M., Kryszczynska, A., Lamy, P., Michalowski, T., Michel, P., Santana-Ros, T., Tanga, P., Vachier, F., Vigan, A., Witasse, O., Yang, B.
Publikováno v:
A&A 633, A65 (2020)
With an estimated diameter in the 320 to 350 km range, (704) Interamnia is the fifth largest main belt asteroid and one of the few bodies that fills the gap in size between the four largest bodies with $D$ > 400 km (Ceres, Vesta, Pallas and Hygiea) a
Externí odkaz:
http://arxiv.org/abs/1911.13049
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
Autor:
Skopal, A., Drechsel, H., Tarasova, T. N., Kato, T., Fujii, M., Teyssier, F., Garde, O., Guarro, J., Edlin, J., Buil, C., Antao, D., Terry, J. N., Lemoult, T., Charbonnel, S., Bohlsen, T., Favaro, A., Graham, K.
Publikováno v:
A&A 569, A112 (2014)
We determine the temporal evolution of the luminosity L(WD), radius R(WD) and effective temperature Teff of the white dwarf (WD) pseudophotosphere of V339 Del from its discovery to around day 40. Another main objective was studying the ionization str
Externí odkaz:
http://arxiv.org/abs/1407.8212
Autor:
Garrel, T., Miroshnichenko, A. S., Danford, S., Charbonnel, S., Houpert, F., Grankin, K. N., Kusakin, A. V.
FF Cam is a variable star near the North celestial pole with hydrogen lines in emission. Its optical variability of ~0.3 mag was discovered by HIPPARCOS. The spectral type assigned to the star in SIMBAD is B9, but its position coincides with a ROSAT
Externí odkaz:
http://arxiv.org/abs/1305.1393
Autor:
Hanuš, J., Ďurech, J., Brož, M., Marciniak, A., Warner, B. D., Pilcher, F., Stephens, R., Behrend, R., Carry, B., Čapek, D., Antonini, P., Audejean, M., Augustesen, K., Barbotin, E., Baudouin, P., Bayol, A., Bernasconi, L., Borczyk, W., Bosch, J. -G., Brochard, E., Brunetto, L., Casulli, S., Cazenave, A., Charbonnel, S., Christophe, B., Colas, F., Coloma, J., Conjat, M., Cooney, W., Correira, H., Cotrez, V., Coupier, A., Crippa, R., Cristofanelli, M., Dalmas, Ch., Danavaro, C., Demeautis, C., Droege, T., Durkee, R., Esseiva, N., Esteban, M., Fagas, M., Farroni, G., Fauvaud, M., Fauvaud, S., Del Freo, F., Garcia, L., Geier, S., Godon, C., Grangeon, K., Hamanowa, H., Heck, N., Hellmich, S., Higgins, D., Hirsch, R., Husarik, M., Itkonen, T., Jade, O., Kamiński, K., Kankiewicz, P., Klotz, A., Koff, R. A., Kryszczyńska, A., Kwiatkowski, T., Laffont, A., Leroy, A., Lecacheux, J., Leonie, Y., Leyrat, C., Manzini, F., Martin, A., Masi, G., Matter, D., Michałowski, J., Michałowski, M. J., Michałowski, T., Michelet, J., Michelsen, R., Morelle, E., Mottola, S., Naves, R., Nomen, J., Oey, J., Ogloza, W., Oksanen, A., Oszkiewicz, D., Pääkkönen, P., Paiella, M., Pallares, H., Paulo, J., Pavic, M., Payet, B., Polińska, M., Polishook, D., Poncy, R., Revaz, Y., Rinner, C., Rocca, M., Roche, A., Romeuf, D., Roy, R., Saguin, H., Salom, P. A., Sanchez, S., Santacana, G., Santana-Ros, T., Sareyan, J. -P., Sobkowiak, K., Sposetti, S., Starkey, D., Stoss, R., Strajnic, J., Teng, J. -P., Tregon, B., Vagnozzi, A., Velichko, F. P., Waelchli, N., Wagrez, K., Wücher, H.
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:
http://arxiv.org/abs/1301.6943
Akademický článek
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Autor:
Dudziński, G., Podlewska-Gaca, E., Bartczak, P., Benseguane, S, Ferrais, M., Jorda, L., Hanuš, J., Vernazza, P., Rambaux, N., Carry, B., Marchis, F., Marsset, M., Viikinkoski, M., Brož, M., Fetick, R., Drouard, A., Fusco, T., Birlan, M., Jehin, E., Berthier, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Dumas, C., Kryszczynska, A., Lamy, P., Le Coroller, H, Marciniak, A., Michalowski, T., Michel, P., Santana-Ros, T., Tanga, P., Vachier, F., Vigan, A., Witasse, O., Yang, Bin, Ďurech, J., Kaasalainen, M., Le Coroller, H., Ševeček, P., Dudzinski, G., DeMeo, F., Durech, J., Grice, J., Gillon, M., Benkhaldoun, Z., Szakats, R., Hirsch, R., Duffard, R., Chapman, A., Maestre, J., Carbognani, Albino, Barghini, D., Gardiol, D., Martino, M. Di, Valsecchi, G., Trivero, P., Buzzoni, A., Rasetti, S., Selvestrel, D., Knapic, C., Londero, E., Zorba, S., Volpicelli, C., Carlo, M. Di, Vaubaillon, J., Marmo, C., Valeri, D., Zanotti, F., Morini, M., Demaria, P., Zanda, B., Bouley, S., Rault, J., Maquet, L., Warner, B., Behrend, R., Asenjo, V., Berger, N., Bronikowska, M., Brothers, T., Charbonnel, S., Colazo, C., Coliac, J.-F., Jones, A., Leroy, A., Melia, R., Molina, D., Nadolny, J., Person, M., Pejcha, O., Riemis, H., Shappee, B., Sobkowiak, K., Soldán, F., Suys, D., Vantomme, J.
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, pp.A65. ⟨10.1051/0004-6361/201936639⟩
Astronomy and Astrophysics-A&A, 2020, 633, A65 (17 p.). ⟨10.1051/0004-6361/201936639⟩
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, A65 (17 p.). ⟨10.1051/0004-6361/201936639⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633 (2), pp.A65. ⟨10.1051/0004-6361/201936639⟩
Astronomy and Astrophysics-A&A, 2020, 633 (2), pp.A65. ⟨10.1051/0004-6361/201936639⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, pp.A65. ⟨10.1051/0004-6361/201936639⟩
Astronomy and Astrophysics-A&A, 2020, 633, A65 (17 p.). ⟨10.1051/0004-6361/201936639⟩
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, A65 (17 p.). ⟨10.1051/0004-6361/201936639⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633 (2), pp.A65. ⟨10.1051/0004-6361/201936639⟩
Astronomy and Astrophysics-A&A, 2020, 633 (2), pp.A65. ⟨10.1051/0004-6361/201936639⟩
Full list of authors: Hanuš, J.; Vernazza, P.; Viikinkoski, M.; Ferrais, M.; Rambaux, N.; Podlewska-Gaca, E.; Drouard, A.; Jorda, L.; Jehin, E.; Carry, B.; Marsset, M.; Marchis, F.; Warner, B.; Behrend, R.; Asenjo, V.; Berger, N.; Bronikowska, M.; B
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::08bbfad857ae5900dc1abd6beecdbeb0
http://hdl.handle.net/10261/229320
http://hdl.handle.net/10261/229320
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
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