The Spectral Energy Distribution and Mass-Loss Rate of the A-Type Supergiant Deneb

@article{Aufdenberg2002TheSE,
  title={The Spectral Energy Distribution and Mass-Loss Rate of the A-Type Supergiant Deneb},
  author={Jason P. Aufdenberg and Peter Hauschildt and Edward A. Baron and Tyler E. Nordgren and A. W. Burnley and Ian D. Howarth and Karl D. Gordon and J. Stansberry},
  journal={The Astrophysical Journal},
  year={2002},
  volume={570},
  pages={344 - 368}
}
A stellar wind module has been developed for the PHOENIX stellar atmosphere code for the purpose of computing non-LTE, line-blanketed, expanding atmospheric structures and detailed synthetic spectra of hot luminous stars with winds. We apply the code to observations of Deneb, for which we report the first positive detections of millimeter and centimeter emission (obtained using the Submillimeter Common-User Bolometric Array and the Very Large Array) as well a strong upper limit on the 870 μm… 

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