Working Group Prof. Klaus Werner - Stellar Atmospheres

Our team works in the field of quantitative spectral analyses of stellar spectra (white dwarfs, neutron stars, etc.) and spectra of accretion disks around compact stellar remnants. For spectral analyses we are utilizing ground- and space-based observatories in a wide wavelength range, from the infrared to the X-ray region of the electromagnetic spectrum.

Group Members

Room and telephone numbers and E-mail adresses

Quantitative spectroscopy of (pre-) white dwarfs and supersoft X-ray sources

Keywords: white dwarfs, PG1159 stars, central stars of planetary nebulae, radiation transport, stellar atmospheres, synthetic spectra, ground and space based observations, GAVO

Thermal emission from neutron stars

Keywords: neutron stars, magnetic fields, neutron star atmospheres, equation of state