Add to ORKGStrong ultraviolet carbon lines were detected in additional white DC (continuous visual spectra) dwarfs using the IUE. These lines are not seen in the ultraviolet spectrum of the cool DC star Stein 2051 B. The bright DA white dwarf LB 3303 has a strong unidentified absorption near lambda 1400
Using newly obtained high-resolution data (R similar to 1 x 10(5)) from the Hubble Space Telescope, ...
Recent research under NASA grant NAG5-971 consisted of the performance of two projects in conjunctio...
Atmospheric parameters for hot DB (helium atmosphere) white dwarfs near effective temperatures of 25...
A high-resolution ultraviolet spectrum of the helium-rich degenerate LDS 678A, obtained with the Int...
Research under NASA Grant NAG5-287 has carried out a number of projects in conjunction with the Inte...
The accretion of planetary debris into the atmospheres of white dwarfs leads to the presence of meta...
White dwarf studies carry significant implications across multiple fields of astrophysics, including...
The atmospheres of very cool, hydrogen-rich white dwarfs (WDs) (T eff < 6000 K) are challenging to m...
The birth rates of various kinds of white dwarf progenitors are estimated and the spectra of two ver...
Two projects in conjunction with the International Ultraviolet Explorer Satellite are discussed. The...
The convective dredge-up of carbon from the interiors of hydrogen-deficient white dwarfs has long be...
Context. The high-quality photometric and astrometric capabilities of the ESA Gaia space mission hav...
We have analyzed FUSE observations of six hot white dwarf stars: four DA white dwarfs with T_eff >= ...
The 21st European Workshop on White Dwarfs was held in Austin, TX from July 23rd to 27th of 2018We p...
Cool white dwarfs with Teff < 6000 K are the remnants of the oldest stars that existed in our Galaxy...
Using newly obtained high-resolution data (R similar to 1 x 10(5)) from the Hubble Space Telescope, ...
Recent research under NASA grant NAG5-971 consisted of the performance of two projects in conjunctio...
Atmospheric parameters for hot DB (helium atmosphere) white dwarfs near effective temperatures of 25...
A high-resolution ultraviolet spectrum of the helium-rich degenerate LDS 678A, obtained with the Int...
Research under NASA Grant NAG5-287 has carried out a number of projects in conjunction with the Inte...
The accretion of planetary debris into the atmospheres of white dwarfs leads to the presence of meta...
White dwarf studies carry significant implications across multiple fields of astrophysics, including...
The atmospheres of very cool, hydrogen-rich white dwarfs (WDs) (T eff < 6000 K) are challenging to m...
The birth rates of various kinds of white dwarf progenitors are estimated and the spectra of two ver...
Two projects in conjunction with the International Ultraviolet Explorer Satellite are discussed. The...
The convective dredge-up of carbon from the interiors of hydrogen-deficient white dwarfs has long be...
Context. The high-quality photometric and astrometric capabilities of the ESA Gaia space mission hav...
We have analyzed FUSE observations of six hot white dwarf stars: four DA white dwarfs with T_eff >= ...
The 21st European Workshop on White Dwarfs was held in Austin, TX from July 23rd to 27th of 2018We p...
Cool white dwarfs with Teff < 6000 K are the remnants of the oldest stars that existed in our Galaxy...
Using newly obtained high-resolution data (R similar to 1 x 10(5)) from the Hubble Space Telescope, ...
Recent research under NASA grant NAG5-971 consisted of the performance of two projects in conjunctio...
Atmospheric parameters for hot DB (helium atmosphere) white dwarfs near effective temperatures of 25...