Add to ORKGThe DAO-type white dwarf LS V+4621 is the hydrogen-rich central star of the possible planetary nebula Sh 2-216. We have taken high-resolution, high-S/N ultraviolet spectra with STIS aboard the HST and FUSE in order to constrain its photospheric parameters. A detailed spectral analysis by means of state-of-the-art NLTE model-atmosphere techniques is presented which includes the determination the individual abundances of iron-group elements
PG1159-035 is the prototype of the PG1159 spectral class which consists of extremely hot hydrogen-de...
The first IUE SWP high-resolution spectral atlas of central stars of planetary nebulae and hot white...
Context.PG 1159-035 is the prototype of the PG 1159 spectral class which consists of extremely hot h...
The far-ultraviolet spectrum of the DAO White Dwarf LS V+4621, the exciting star of the possible pla...
Context. We perform a comprehensive spectral analysis of LS V +46°21 in order to compare its photo...
The determination of effective temperatures of very hot central stars (Teff>70000K) by model atmosph...
The birth rates of various kinds of white dwarf progenitors are estimated and the spectra of two ver...
We report early FUSE observations of the very hot DA white dwarfs PG1342+444 and REJ0558-371. Detect...
We present an abundance analysis of the far-ultraviolet (905--1187 A) spectrum of the subdwarf B sta...
‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing....
High-resolution UV spectra, obtained with HST and FUSE, enable us to analyse hot hydrogen-rich centr...
We present a detailed spectroscopic analysis of the hot DA white dwarf G191-B2B, using the best sign...
We have analyzed FUSE observations of six hot white dwarf stars: four DA white dwarfs with T_eff >= ...
We present results from our analysis of a sample of DA white dwarfs having effective temperature bel...
PG 1159 stars are hot, hydrogen-deficient (pre-) white dwarfs with atmospheres mainly composed of he...
PG1159-035 is the prototype of the PG1159 spectral class which consists of extremely hot hydrogen-de...
The first IUE SWP high-resolution spectral atlas of central stars of planetary nebulae and hot white...
Context.PG 1159-035 is the prototype of the PG 1159 spectral class which consists of extremely hot h...
The far-ultraviolet spectrum of the DAO White Dwarf LS V+4621, the exciting star of the possible pla...
Context. We perform a comprehensive spectral analysis of LS V +46°21 in order to compare its photo...
The determination of effective temperatures of very hot central stars (Teff>70000K) by model atmosph...
The birth rates of various kinds of white dwarf progenitors are estimated and the spectra of two ver...
We report early FUSE observations of the very hot DA white dwarfs PG1342+444 and REJ0558-371. Detect...
We present an abundance analysis of the far-ultraviolet (905--1187 A) spectrum of the subdwarf B sta...
‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing....
High-resolution UV spectra, obtained with HST and FUSE, enable us to analyse hot hydrogen-rich centr...
We present a detailed spectroscopic analysis of the hot DA white dwarf G191-B2B, using the best sign...
We have analyzed FUSE observations of six hot white dwarf stars: four DA white dwarfs with T_eff >= ...
We present results from our analysis of a sample of DA white dwarfs having effective temperature bel...
PG 1159 stars are hot, hydrogen-deficient (pre-) white dwarfs with atmospheres mainly composed of he...
PG1159-035 is the prototype of the PG1159 spectral class which consists of extremely hot hydrogen-de...
The first IUE SWP high-resolution spectral atlas of central stars of planetary nebulae and hot white...
Context.PG 1159-035 is the prototype of the PG 1159 spectral class which consists of extremely hot h...