作者: Lynne A. Hillenbrand , Stephen E. Strom , Frederick J. Vrba , Jocelyn Keene
DOI: 10.1086/171819
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摘要: The proposition that Herbig Ae/Be stars are young intermediate mass surrounded by optically thick accretion disks is explored. From a study of 47 such objects, subset 30 identified whose spectral energy distributions can be interpreted convincingly in terms pre-main sequence massive circumstellar disks. Constraints on the physical properties disks, as size, mass, rate, lifetime, and radial structure derived from photometric data.