The O VIII phenomenon describes the occurrence of ultra-high ionization absorption lines of the CNO elements (e.g. O VIII, N VII, C VI, and even Ne X) in the optical spectra hot of DO WDs
We present a small collection of FUSE spectra representative of the main spectral classes found in w...
Original paper can be found at: http://astrosociety.org/pubs/cs/328.html Copyright ASPWe present hig...
We performed a new analysis of UV and optical spectra of KPD 0005+5106. We find T(sub eff) = 200000 ...
About a dozen hot white dwarfs with effective temperatures T(sub eff) = 65000120000 K exhibit unusua...
We have analyzed FUSE observations of six hot white dwarf stars: four DA white dwarfs with T_eff >= ...
Aims. Our aim is to gain new insights into highly ionized gas towards nearby hot white dwarfs (WDs)....
International audience Aims: Our aim is to gain new insights into highly ionized gas towards nearby ...
We report early FUSE observations of the very hot DA white dwarfs PG1342+444 and REJ0558-371. Detect...
Aims. Our aim is to gain new insights into highly ionized gas towards nearby hot white dwarfs (WDs)...
For the first time, we have identified $\ion{Ne}{viii}$ absorption lines in far-UV spectra of the ho...
We present a phenomenological study of highly ionised, non-photospheric absorption features in high ...
‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing....
Context. About 10% of all stars exhibit absorption lines of ultra-highly excited (UHE) metals (e.g.,...
About a dozen hot white dwarfs with effective temperatures Teff = 65 000−120 000 K exhibit unusual a...
We have used Far Ultraviolet Spectroscopic Explorer (FUSE) to obtain a series of 13 observations of ...
We present a small collection of FUSE spectra representative of the main spectral classes found in w...
Original paper can be found at: http://astrosociety.org/pubs/cs/328.html Copyright ASPWe present hig...
We performed a new analysis of UV and optical spectra of KPD 0005+5106. We find T(sub eff) = 200000 ...
About a dozen hot white dwarfs with effective temperatures T(sub eff) = 65000120000 K exhibit unusua...
We have analyzed FUSE observations of six hot white dwarf stars: four DA white dwarfs with T_eff >= ...
Aims. Our aim is to gain new insights into highly ionized gas towards nearby hot white dwarfs (WDs)....
International audience Aims: Our aim is to gain new insights into highly ionized gas towards nearby ...
We report early FUSE observations of the very hot DA white dwarfs PG1342+444 and REJ0558-371. Detect...
Aims. Our aim is to gain new insights into highly ionized gas towards nearby hot white dwarfs (WDs)...
For the first time, we have identified $\ion{Ne}{viii}$ absorption lines in far-UV spectra of the ho...
We present a phenomenological study of highly ionised, non-photospheric absorption features in high ...
‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing....
Context. About 10% of all stars exhibit absorption lines of ultra-highly excited (UHE) metals (e.g.,...
About a dozen hot white dwarfs with effective temperatures Teff = 65 000−120 000 K exhibit unusual a...
We have used Far Ultraviolet Spectroscopic Explorer (FUSE) to obtain a series of 13 observations of ...
We present a small collection of FUSE spectra representative of the main spectral classes found in w...
Original paper can be found at: http://astrosociety.org/pubs/cs/328.html Copyright ASPWe present hig...
We performed a new analysis of UV and optical spectra of KPD 0005+5106. We find T(sub eff) = 200000 ...