Zobrazeno 1 - 10
of 119
pro vyhledávání: '"Morelle E."'
Autor:
Hanuš, J., Delbo', M., Alí-Lagoa, V., Bolin, B., Jedicke, R., Ďurech, J., Cibulková, H., Pravec, P., Kušnirák, P., Behrend, R., Marchis, F., Antonini, P., Arnold, L., Audejean, M., Bachschmidt, M., Bernasconi, L., Brunetto, L., Casulli, S., Dymock, R., Esseiva, N., Esteban, M., Gerteis, O., de Groot, H., Gully, H., Hamanowa, H., Krafft, P., Lehký, M., Manzini, F., Michelet, J., Morelle, E., Oey, J., Pilcher, F., Reignier, F., Roy, R., Salom, P. A., Warner, B. D.
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
Externí odkaz:
http://arxiv.org/abs/1707.05507
Autor:
de Miguel, E., Patterson, J., Cejudo, D., Ulowetz, J., Jones, J. L., Boardman, J., Barret, D., Koff, R., Stein, W., Campbell, T., Vanmunster, T., Menzies, K., Slauson, D., Goff, W., Roberts, G., Morelle, E., Dvorak, S., Hambsch, F. -J., Starkey, D., Collins, D., Costello, M., Cook, M. J., Oksanen, A., Lemay, D., Cook, L. M., Ogmen, Y., Richmond, M., Kemp, J.
We report the results of a long campaign of time-series photometry on the nova-like variable UX Ursae Majoris during 2015. It spanned 150 nights, with ~1800 hours of coverage on 121 separate nights. The star was in its normal `high state' near magnit
Externí odkaz:
http://arxiv.org/abs/1512.08687
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:
Tanga, P., Carry, B., Colas, F., Delbo, M., Matter, A., Hanus, J., Lagoa, V. Ali, Andrei, A. H., Assafin, M., Audejean, M., Behrend, R., Camargo, J. I. B., Carbognani, A., Reyes, M. Cedres, Conjat, M., Cornero, N., Coward, D., Crippa, R., Fantin, E. de Ferra, Devogele, M., Dubos, G., Frappa, E., Gillon, M., Hamanowa, H., Jehin, E., Klotz, A., Kryszczynska, A., Lecacheux, J., Leroy, A., Manfroid, J., Manzini, F., Maquet, L., Morelle, E., Mottola, S., Polinska, M., Roy, R., Todd, M., Vachier, F., Hernandez, C. Vera, Wiggins, P.
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:
http://arxiv.org/abs/1502.00460
Autor:
Carry, B., Matter, A., Scheirich, P., Pravec, P., Molnar, L., Mottola, S., Carbognani, A., Jehin, E., Marciniak, A., Binzel, R. P., DeMeo, F. E., Birlan, M., Delbo, M., Barbotin, E., Behrend, R., Bonnardeau, M., Colas, F., Farissier, P., Fauvaud, M., Fauvaud, S., Gillier, C., Gillon, M., Hellmich, S., Hirsch, R., Leroy, A., Manfroid, J., Montier, J., Morelle, E., Richard, F., Sobkowiak, K., Strajnic, J., Vachier, F.
In understanding the composition and internal structure of asteroids, their density is perhaps the most diagnostic quantity. We aim here to characterize the surface composition, mutual orbit, size, mass, and density of the small main-belt binary aste
Externí odkaz:
http://arxiv.org/abs/1411.0872
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
Autor:
Hanuš, J., Delbo’, M., Alí-Lagoa, V., Bolin, B., Jedicke, R., Ďurech, J., Cibulková, H., Pravec, P., Kušnirák, P., Behrend, R., Marchis, F., Antonini, P., Arnold, L., Audejean, M., Bachschmidt, M., Bernasconi, L., Brunetto, L., Casulli, S., Dymock, R., Esseiva, N., Esteban, M., Gerteis, O., de Groot, H., Gully, H., Hamanowa, Hiroko, Hamanowa, Hiromi, Krafft, P., Lehký, M., Manzini, F., Michelet, J., Morelle, E., Oey, J., Pilcher, F., Reignier, F., Roy, R., Salom, P.A., Warner, B.D.
Publikováno v:
In Icarus 1 January 2018 299:84-96
Autor:
Carry, B., Matter, A., Scheirich, P., Pravec, P., Molnar, L., Mottola, S., Carbognani, A., Jehin, E., Marciniak, A., Binzel, R.P., DeMeo, F.E., Birlan, M., Delbo, M., Barbotin, E., Behrend, R., Bonnardeau, M., Colas, F., Farissier, P., Fauvaud, M., Fauvaud, S., Gillier, C., Gillon, M., Hellmich, S., Hirsch, R., Leroy, A., Manfroid, J., Montier, J., Morelle, E., Richard, F., Sobkowiak, K., Strajnic, J., Vachier, F.
Publikováno v:
In Icarus 1 March 2015 248:516-525
Publikováno v:
Fachtagung "Experimentelle Strömungsmechanik", 06.-08.09.2022, Ilmenau, Germany
Fachtagung “Experimentelle Strömungsmechanik", 06.-08.09.2022, Ilmenau, Germany
Fachtagung “Experimentelle Strömungsmechanik", 06.-08.09.2022, Ilmenau, Germany
Various physicochemical properties play a decisive role in the evaluation of foods, influencing taste, odor, texture and mouthfeel when the food is distorted. Therefore, rheological investiga- tions of foods are used in product development to specifi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::45be53c7e7e3d7d7f64854bc025bc81e
https://www.hzdr.de/publications/Publ-35546-2
https://www.hzdr.de/publications/Publ-35546-2
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