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pro vyhledávání: '"Rigliaco, M. Langlois E."'
Autor:
Sissa, E., Olofsson, J., Vigan, A., Augereau, J. C., D'Orazi, V., Desidera, S., Gratton, R., Rigliaco, M. Langlois E., Boccaletti, A., Kral, Q., Lazzoni, C., Mesa, D., Messina, S., Sezestre, E., Thébault, P., Zurlo, A., Bhowmik, T., Bonnefoy, M., Chauvin, G., Feldt, M., Hagelberg, J., Lagrange, A. -M., Janson, M., Maire, A. -L., Ménard, F., Schlieder, J., Schmidt, T., Szulágyi, J., Stadler, E., Deboulbé, D. Maurel A., Feautrier, P., Ramos, J., Rigal, R.
Publikováno v:
A&A 613, L6 (2018)
Debris disks are usually detected through the infrared excess over the photospheric level of their host star. The most favorable stars for disk detection are those with spectral types between A and K, while the statistics for debris disks detected ar
Externí odkaz:
http://arxiv.org/abs/1804.02882
