The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

Autor: Valerio Nascimbeni, J. Lecacheux, Toni Santana-Ros, Agustín Sánchez-Lavega, Pablo Santos-Sanz, L. Nerli, D. T. Koseoglu, Frédéric Vachier, V. Peris, Przemyslaw Bartczak, R. Komžík, Eda Sonbas, Cs. Kiss, Gábor Marton, C. Ries, Yavuz Güney, Marcelo Assafin, Martina Maestripieri, Josselin Desmars, T. G. Mueller, Osman Demircan, O. Erece, V. Granata, A. R. Gomes-Júnior, Francesco Marzari, Ulrich Hopp, Cahit Yeşilyaprak, N. Paschalis, A. Campo Bagatin, B. Gaehrken, Paolo Bacci, V. Tsamis, O. Satir, F. Martinelli, F. L. Rommel, Santiago Pérez-Hoyos, F. Ciabattari, R. Iglesias-Marzoa, Stefano Mottola, Ricardo Hueso, Julio Camargo, Herman Mikuz, Françoise Roques, Mohammad Shameoni Niaei, Mauro Bachini, Vassilis Charmandaris, Jose Luis Ortiz, A. Takácsné Farkas, András Pál, A. Carbognani, L. Tzouganatos, Giuseppe Leto, Aleksandar Cikota, G. Benedetti-Rossi, Roberto Vieira-Martins, Nicolás Morales, José M. Madiedo, Bruno Sicardy, Róbert Szakáts, B. E. Morgado, Theodor Pribulla, Estela Fernández-Valenzuela, M. Butkiewicz-Bąk, Afşar Kabaş, Alvaro Alvarez-Candal, Giacomo Succi, Jérôme Berthier, J. Alikakos, Ç. Püsküllü, Kamil Hornoch, W. Beisker, E. Meza, Stefan Cikota, T. Ozisik, E. Varga-Verebélyi, J. M. Christille, J. C. Guirado, Grzegorz Dudziński, L. Mazzei, J. M. Ohlert, Rene Duffard, Raoul Behrend, S. Kalkan, A. Marciniak, N. Karaman, S. Hellmich, Kosmas Gazeas, Victor Ali-Lagoa, Ozan Ünsalan, Felipe Braga-Ribas, François Colas, Petr Pravec, Diane Berard

Publikováno v: RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Nature
Nature, 2017, 550 (7675), pp.219-223. ⟨10.1038/nature24051⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Nature, Nature Publishing Group, 2017, 550 (7675), pp.219-223. ⟨10.1038/nature24051⟩

Ortiz, José Luis et. al.
Haumea-one of the four known trans-Neptunian dwarf planets- is a very elongated and rapidly rotating body1-3. In contrast to other dwarf planets4-6, its size, shape, albedo and density are not well constrained. The Cent

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa292d0be284f3008c5a229e471447f1
http://hdl.handle.net/10045/70230

Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.