TLUSTY: Stellar Atmospheres, Accretion Disks, and Spectroscopic Diagnostics

Details TLUSTY: Stellar Atmospheres, Accretion Disks, and Spectroscopic Diagnostics TLUSTY: Stellar Atmospheres, Accretion Disks, and Spectroscopic Diagnostics

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ascl.soft09021h&link_type=abstract

Astrophysics Source Code Library, record ascl:1109.021

Astronomy and Astrophysics

Astrophysics

Scientific paper

TLUSTY is a user-oriented package written in FORTRAN77 for modeling stellar atmospheres and accretion disks and wide range of spectroscopic diagnostics. In the program's 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.

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