Model atoms - PowerPoint PPT Presentation

NLTE Model Atmospheres for Super-Soft X- ray Sources

NLTE Model Atmospheres for Super-Soft X- ray Sources. Thomas Rauch, Klaus Werner and the GAVO and AstroGrid-D Teams. Spectral Energy Distributions for Hot Stars. The nebular information indicates that the spectrum of the star deviates considerably from a blackbody . Author in 2008!.

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524 views • 32 slides

Spectral Analysis in the VO

Spectral Analysis in the VO. Thomas Rauch, Iliya Nickelt and the GAVO and AstroGrid-D Teams. Spectral Energy Distributions for Hot Stars. The nebular information indicates that the spectrum of the star deviates considerably from a blackbody . Author in 2008!.

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362 views • 18 slides

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