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pro vyhledávání: '"Navas, G. Y."'
Autor:
Morgado, B., Benedetti-Rossi, G., Gomes-Júnior, A. R., Assafin, M., Lainey, V., Vieira-Martins, R., Camargo, J. I. B., Braga-Ribas, F., Boufleur, R. C., Fabrega, J., Machado, D. I., Maury, A., Trabuco, L. L., de Barros, J. R., Cacella, P., Crispim, A., Jaques, C., Navas, G. Y., Pimentel, E., Rommel, F. L., de Santana, T., Schoenell, W., Sfair, R., Winter, O. C.
Publikováno v:
A&A, 626, L4 (2019)
Context. Bright stellar positions are now known with an uncertainty below 1 mas thanks to Gaia DR2. Between 2019-2020, the Galactic plane will be the background of Jupiter. The dense stellar background will lead to an increase in the number of occult
Externí odkaz:
http://arxiv.org/abs/1905.12520