Supergiant B[e] with HDUST
The Supergiant B[e] with HDUST model was created by A. Domiciano de Souza.
It is described in the following references:
Grid of Supergiant B[e] Models from HDUST Radiative Transfer
A. Domiciano de Souza and A. C. Carciofi
in Circumstellar Dynamics at High Resolution
A. Carciofi and Th. Rivinius eds.
ASP Conference Proceedings 464, 149 (2012)
Non-LTE Monte Carlo Radiative Transfer. I. The Thermal Properties of Keplerian Disks around Classical Be Stars
A. C. Carciofi and J. E. Bjorkman
ApJ 639 (2), 1081-1094 (2006)
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AMHRA's Supergiant B[e] with HDUST service can be acknowledged by:
- And citing the two references above.