Accurate determination of accretion and photospheric parameters in Young Stellar Objects: the case of two candidate old disks in the Orion Nebula Cluster
C. F. Manara (1), G. Beccari (1), N. Da Rio (2), G. De Marchi (2), A. Natta (3,4), L. Ricci (5), M. Robberto (6), L. Testi (1,3,7) ((1) ESO-Garching, (2) ESA-ESTEC, (3) INAF-Arcetri, (4) Dublin Institute for Advanced Studies, (5) Caltech, (6) STScI, (7) Excellence Cluster Universe)
http://xxx.yukawa.kyoto-u.ac.jp/abs/1307.8118
