Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

Autor: Marciniak, A., Ďurech, J., Alí-Lagoa, V., Ogłoza, W., Szakáts, R., Müller, T. G., Molnár, L., Pál, A., Monteiro, F., Arcoverde, P., Behrend, R., Benkhaldoun, Z., Bernasconi, L., Bosch, J., Brincat, S., Brunetto, L., Bąk, M. Butkiewicz, Del Freo, F., Duffard, R., Evangelista-Santana, M., Farroni, G., Fauvaud, S., Fauvaud, M., Ferrais, M., Geier, S., Golonka, J., Grice, J., Hirsch, R., Horbowicz, J., Jehin, E., Julien, P., Kalup, Cs., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kecskeméthy, V., Kim, D. -H., Kim, M. -J., Konstanciak, I., Krajewski, J., Kudak, V., Kulczak, P., Kundera, T., Lazzaro, D., Manzini, F., Medeiros, H., Michimani-Garcia, J., Morales, N., Nadolny, J., Oszkiewicz, D., Pakštienė, E., Pawłowski, M., Perig, V., Pilcher, F., Pinel, P., Podlewska-Gaca, E., Polakis, T., Richard, F., Rodrigues, T., Rondon, E., Roy, R., Sanabria, J. J., Santana-Ros, T., Skiff, B., Skrzypek, J., Sobkowiak, K., Sonbas, E., Stachowski, G., Strajnic, J., Trela, P., Tychoniec, Ł., Urakawa, S., Verebelyi, E., Wagrez, K., Żejmo, M., Żukowski, K.

Publikováno v: A&A 654, A87 (2021)

Results from the TESS mission showed that previous studies strngly underestimated the number of slow rotators, revealing the importance of studying those asteroids. For most slowly rotating asteroids (P > 12), no spin and shape model is available bec

Externí odkaz: http://arxiv.org/abs/2109.00463

Photometric survey, modelling, and scaling of long-period and low-amplitude asteroids

Autor: Marciniak, A., Bartczak, P., Müller, T., Sanabria, J. J., Alí-Lagoa, V., Antonini, P., Behrend, R., Bernasconi, L., Bronikowska, M., Bąk, M. Butkiewicz, Cikota, A., Crippa, R., Ditteon, R., Dudziński, G., Duffard, R., Dziadura, K., Fauvaud, S., Geier, S., Hirsch, R., Horbowicz, J., Hren, M., Jerosimic, L., Kamiński, K., Kankiewicz, P., Konstanciak, I., Korlevic, P., Kosturkiewicz, E., Kudak, V., Manzini, F., Morales, N., Murawiecka, M., Ogłoza, W., Oszkiewicz, D., Pilcher, F., Polakis, T., Poncy, R., Santana-Ros, T., Siwak, M., Skiff, B., Sobkowiak, K., Stoss, R., Żejmo, M., Żukowski, K.

The available set of spin and shape modelled asteroids is strongly biased against slowly rotating targets and those with low lightcurve amplitudes. As a consequence of these selection effects, the current picture of asteroid spin axis distribution, r

Externí odkaz: http://arxiv.org/abs/1711.01893