Context. We perform a comprehensive spectral analysis of LS V +46°21 in order to compare its photospheric properties to theoretical predictions from stellar evolution theory as well as from diffusion calculations. Aims. LS V +46°21 is the DAO-type central star of the planetary nebula Sh 2-21
Context. About 2500 planetary nebulae are known in our Galaxy but only 224 have central stars with r...
We analyze the far-UV/UV spectra of four central stars of planetary nebulae (CSPNs) with strong wind...
The UV spectrum of PC 11 is found to show variations in the strength of the O III] 1666 Angstrom, N ...
The DAO-type white dwarf LS V+4621 is the hydrogen-rich central star of the possible planetary nebul...
The first IUE SWP high-resolution spectral atlas of central stars of planetary nebulae and hot white...
The far-ultraviolet spectrum of the DAO White Dwarf LS V+4621, the exciting star of the possible pla...
Context. Spectral analyses of hot, compact stars with non-local thermodynamical equilibrium (NLTE) m...
‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing....
We present Gemini-South observations of nine faint and extended planetary nebulae (PNe). Using direc...
International audienceWe present a comprehensive study of the Magellanic Cloud planetary nebula SMP ...
Aims. The evolution of central stars of planetary nebulae was so far documented in just a few cases....
Aims. We discuss the status of the A-type component of the binary central star in the peculiar plane...
Context.The Sloan Digital Sky Survey Data Release 4 has provided spectra of several new PG 1159 sta...
We analyze an HST/STIS ultraviolet spectrum of the young brown dwarf 2MASSW J1207334-393254, a membe...
We present a detailed study of the suspected Chemically Peculiar star HD 207538 based on high resolu...
Context. About 2500 planetary nebulae are known in our Galaxy but only 224 have central stars with r...
We analyze the far-UV/UV spectra of four central stars of planetary nebulae (CSPNs) with strong wind...
The UV spectrum of PC 11 is found to show variations in the strength of the O III] 1666 Angstrom, N ...
The DAO-type white dwarf LS V+4621 is the hydrogen-rich central star of the possible planetary nebul...
The first IUE SWP high-resolution spectral atlas of central stars of planetary nebulae and hot white...
The far-ultraviolet spectrum of the DAO White Dwarf LS V+4621, the exciting star of the possible pla...
Context. Spectral analyses of hot, compact stars with non-local thermodynamical equilibrium (NLTE) m...
‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing....
We present Gemini-South observations of nine faint and extended planetary nebulae (PNe). Using direc...
International audienceWe present a comprehensive study of the Magellanic Cloud planetary nebula SMP ...
Aims. The evolution of central stars of planetary nebulae was so far documented in just a few cases....
Aims. We discuss the status of the A-type component of the binary central star in the peculiar plane...
Context.The Sloan Digital Sky Survey Data Release 4 has provided spectra of several new PG 1159 sta...
We analyze an HST/STIS ultraviolet spectrum of the young brown dwarf 2MASSW J1207334-393254, a membe...
We present a detailed study of the suspected Chemically Peculiar star HD 207538 based on high resolu...
Context. About 2500 planetary nebulae are known in our Galaxy but only 224 have central stars with r...
We analyze the far-UV/UV spectra of four central stars of planetary nebulae (CSPNs) with strong wind...
The UV spectrum of PC 11 is found to show variations in the strength of the O III] 1666 Angstrom, N ...
DOI
Add to ORKG