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We calculated plane-parallel, chemically homogeneous model-atmospheres in hydrostatic and radiative equilibrium with the Tübingen Non-local thermodynamic equilibrium (NLTE) Model Atmosphere Package (TMAP). Model atoms were taken from the Tübingen Model Atom Database (TMAD). For further information about TMAP and TMAD see Werner et al. (2003, 2012) and Rauch & Deetjen (2003), respectivley.

On this website we presented our currently best stellar model-atmosphere (red) for the sdOB Feige110 (Teff = 47250 K, log (g / cm/s2) = 6.00).

In the plot below we show the complete energy distribution of the far ultraviolet (FUV) and you will find some information about the observation.
To scroll in the plots, press <SHIFT> and use your mouse wheel.

FUSE

The observation which is shown here is available under the Observation Id M1080801, and P1044301. The reached resolving power for FUSE is for the given wavelength range between 15000 and 20000.