A mid-term astrometric and photometric study of trans-Neptunian object (90482) Orcus

From time series CCD observations of a fixed and large star field that contained the binary trans-Neptunian object (90482) Orcus (formerly 2004 DW), taken during a period of 33 days, we have been able to derive high-precision relative astrometry and photometry of the Orcus system with respect to bac...

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Detalles Bibliográficos
Autores principales: Ortiz, J. L., Cikota, A., Cikota, S., Hestroffer, D., Thirouin, A., Morales, N., Duffard, R., Gil-Hutton, Ricardo, Santos Sanz, P., Cueva, I. de la
Formato: Articulo
Lenguaje:Inglés
Publicado: 2010
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/101535
https://ri.conicet.gov.ar/11336/29461
https://www.aanda.org/articles/aa/abs/2011/01/aa15309-10/aa15309-10.html
Aporte de:SEDICI (UNLP) de Universidad Nacional de La Plata Ver origen

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