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Ivan Hubeny & Thierry Lanz



University Of Arizona Steward Observatory

Observatoire de la Cote d'Azur


A user-oriented package for modeling stellar atmospheres and accretion disks
and for stellar spectroscopic diagnostics

The present set of computer programs is a package designed to accomplish a wide range of spectroscopic diagnostics. In its maximum configuration, the user may start from scratch and calculate a model atmosphere of a chosen degree of complexity, and end with a synthetic spectrum in a wavelength region of interest for an arbitrary stellar rotation and an arbitrary instrumental profile. The user may also model the vertical structure of annuli of an accretion disk.