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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 DAO-type exciting central star of Abell 35 (Teff = 80000 K, log (g / cm/s2) = 7.20).

In the plots below we show the complete energy distribution from the far ultraviolet (FUV) till to the ultraviolet (UV). Each plot describes a typical wavelength range (FUV and UV) and you will find some information about the observation.
To scroll in the plots, press <SHIFT> and use your mouse wheel.

FUSE

The observation (P1330101000) which is shown here was obtained from the MAST archive and rectified by Löbling et al. (in prep.)


STIS

The observation which is shown here is available under the Observation Id O4GT02010, O4GT02020, O4GT02030, and O4GT02040 in the MAST archive.