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2012ApJ...753...14S - Astrophys. J., 753, 14 (2012/July-1)
First light LBT AO images of HR 8799 bcde at 1.6 and 3.3 µm: new discrepancies between young planets and old brown dwarfs.
SKEMER A.J., HINZ P.M., ESPOSITO S., BURROWS A., LEISENRING J., SKRUTSKIE M., DESIDERA S., MESA D., ARCIDIACONO C., MANNUCCI F., RODIGAS T.J., CLOSE L., McCARTHY D., KULESA C., AGAPITO G., APAI D., ARGOMEDO J., BAILEY V., BOUTSIA K., BRIGUGLIO R., BRUSA G., BUSONI L., CLAUDI R., EISNER J., FINI L., FOLLETTE K.B., GARNAVICH P., GRATTON R., GUERRA J.C., HILL J.M., HOFFMANN W.F., JONES T., KREJNY M., MALES J., MASCIADRI E., MEYER M.R., MILLER D.L., MORZINSKI K., NELSON M., PINNA E., PUGLISI A., QUANZ S.P., QUIROS-PACHECO F., RICCARDI A., STEFANINI P., VAITHEESWARAN V., WILSON J.C. and XOMPERO M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): brown dwarfs - instrumentation: adaptive optics - planetary systems - planets and satellites: atmospheres - stars: individual: HR 8799
Simbad objects: 6
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