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2012ApJ...751..118C - Astrophys. J., 751, 118 (2012/June-1)
A possible detection of occultation by a proto-planetary clump in GM Cephei.
CHEN W.P., HU S.C.-L., ERRMANN R., ADAM C., BAAR S., BERNDT A., BUKOWIECKI L., DIMITROV D.P., EISENBEISS T., FIEDLER S., GINSKI C., GRAFE C., GUO J.K., HOHLE M.M., HSIAO H.Y., JANULIS R., KITZE M., LIN H.C., LIN C.S., MACIEJEWSKI G., MARKA C., MARSCHALL L., MOUALLA M., MUGRAUER M., NEUHAUSER R., PRIBULLA T., RAETZ S., ROLL T., SCHMIDT E., SCHMIDT J., SCHMIDT T.O.B., SEELIGER M., TREPL L., BRICENO C., CHINI R., JENSEN E.L.N., NIKOGOSSIAN E.H., PANDEY A.K., SPERAUSKAS J., TAKAHASHI H., WALTER F.M., WU Z.-Y. and ZHOU X.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): occultations - planets and satellites: formation - protoplanetary disks - stars: individual: GM Cephei - stars: pre-main sequence - stars: variables: T Tauri, Herbig Ae/Be
Simbad objects: 7
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