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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 DO-type white dwarf RE 0503-289 (Teff = 70000 K, log (g / cm/s2) = 7.50).

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

EUVE

The observation which is shown here is available under the Observation Id mct_0501-2858__9310202237N in the MAST archive.


FUSE

The observation which is shown here is a combination by Werner et al. (2012) from three separate observations (M1123601, M1124201, and P2041601). All observations are available in the MAST archive.


STIS

The observation which is shown here is available under the Observation Id OC7N01010, OC7N01020, OC7N01030, and OC7N01040 in the MAST archive.


UVES

The observation which is shown here is from SPY - The ESO Supernovae Type Ia Survey (Napiwotzki et al. 2001, 2003).