Add to ORKGHD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this group and also the only one known spectroscopic binary. The complete paper will appear in the "Publications of the Astronomical Society of the Pacific".Asociación Argentina de Astronomí
“The original publication is available at www.springerlink.com” Copyright Springer [Full text of thi...
We started a new project which aims to find compact hot subdwarf binaries at low Galactic latitudes...
The estimation of the binary fraction of hot subdwarfs is key to shed light on the different evoluti...
HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this gro...
We report the discovery of the first hot subdwarf B (sdB) star with a massive compact companion in a...
Research into hot subdwarf stars is progressing rapidly. We present recent important discoveries. Fi...
We review the X-ray observations of hot subdwarf stars. While no X-ray emission has been detected ye...
Helium-rich subdwarf B (He-sdB) stars form a very small fraction of the population of hot subdwarf...
We report the discovery of the first short-period binary in which a hot subdwarf star (sdOB) filled ...
In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the av...
Research into hot subdwarf stars is progressing rapidly. We present recent important discoveries. Fi...
With Hipparcos we have derived the astrometric distance of three hot subdwarf stars (sdO): BD +37 f...
We report the discovery of the ultracompact hot subdwarf (sdOB) binary OWJ074106.0-294811.0 with an ...
We report the discovery of a bright (mV = 11.6 mag), eclipsing, hot subdwarf binary of spectral type...
Hot subluminous stars of spectral type B and O are core helium-burning stars at the blue end of the ...
“The original publication is available at www.springerlink.com” Copyright Springer [Full text of thi...
We started a new project which aims to find compact hot subdwarf binaries at low Galactic latitudes...
The estimation of the binary fraction of hot subdwarfs is key to shed light on the different evoluti...
HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this gro...
We report the discovery of the first hot subdwarf B (sdB) star with a massive compact companion in a...
Research into hot subdwarf stars is progressing rapidly. We present recent important discoveries. Fi...
We review the X-ray observations of hot subdwarf stars. While no X-ray emission has been detected ye...
Helium-rich subdwarf B (He-sdB) stars form a very small fraction of the population of hot subdwarf...
We report the discovery of the first short-period binary in which a hot subdwarf star (sdOB) filled ...
In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the av...
Research into hot subdwarf stars is progressing rapidly. We present recent important discoveries. Fi...
With Hipparcos we have derived the astrometric distance of three hot subdwarf stars (sdO): BD +37 f...
We report the discovery of the ultracompact hot subdwarf (sdOB) binary OWJ074106.0-294811.0 with an ...
We report the discovery of a bright (mV = 11.6 mag), eclipsing, hot subdwarf binary of spectral type...
Hot subluminous stars of spectral type B and O are core helium-burning stars at the blue end of the ...
“The original publication is available at www.springerlink.com” Copyright Springer [Full text of thi...
We started a new project which aims to find compact hot subdwarf binaries at low Galactic latitudes...
The estimation of the binary fraction of hot subdwarfs is key to shed light on the different evoluti...