About a third of the hot subdwarfs of spectral type B, which are mostly core-helium burning objects on the extreme horizontal branch, are found in close binaries with cool, low-mass stellar, substellar, or white dwarf companions. They can show light variations due to different phenomena. We used light curves from the Transiting Exoplanet Survey Satellite and the \textit{K2} space mission to look for more sdB binaries. Their light curves can be used to study the hot subdwarf primaries and their companions and get orbital, atmospheric, and absolute parameters for those systems. By classifying the light variations and combining this with the fit of the spectral energy distribution, the distance derived by the parallaxes obtained by \textit{Gai...
Hot subdwarf stars are evolved, subluminous, helium-burning stars, most likely formed when red-giant...
Hot subdwarfs (sdO/Bs) are the helium-burning cores of red giants, which have lost almost all of the...
We give an update of the results of a campaign to obtain orbital solutions of subdwarf B stars from ...
Context. About a third of the hot subdwarfs of spectral type B (sdBs), which are mostly core-helium-...
We have measured the orbital parameters of seven close binaries, including six new objects,in a radi...
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...
Item does not contain fulltextThe project Massive Unseen Companions to Hot Faint Underluminous Stars...
The origin of hot subdwarf B stars (sdBs) is still unclear. About half of the known sdBs are in clos...
The atmospheric parameters of 34 hot subdwarf B stars have been obtained using a combination of 61 ...
We started a new project which aims to find compact hot subdwarf binaries at low Galactic latitudes...
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...
The origin of hot subdwarf B stars (sdBs) is still unclear. About half of the known sdBs are in clo...
A large fraction of the sdB stars reside in short period binaries. It is therefore clear that binary...
Contains fulltext : 35377.pdf (preprint version ) (Open Access)We give an update o...
Hot subdwarf stars are evolved, subluminous, helium-burning stars, most likely formed when red-giant...
Hot subdwarfs (sdO/Bs) are the helium-burning cores of red giants, which have lost almost all of the...
We give an update of the results of a campaign to obtain orbital solutions of subdwarf B stars from ...
Context. About a third of the hot subdwarfs of spectral type B (sdBs), which are mostly core-helium-...
We have measured the orbital parameters of seven close binaries, including six new objects,in a radi...
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...
Item does not contain fulltextThe project Massive Unseen Companions to Hot Faint Underluminous Stars...
The origin of hot subdwarf B stars (sdBs) is still unclear. About half of the known sdBs are in clos...
The atmospheric parameters of 34 hot subdwarf B stars have been obtained using a combination of 61 ...
We started a new project which aims to find compact hot subdwarf binaries at low Galactic latitudes...
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...
The origin of hot subdwarf B stars (sdBs) is still unclear. About half of the known sdBs are in clo...
A large fraction of the sdB stars reside in short period binaries. It is therefore clear that binary...
Contains fulltext : 35377.pdf (preprint version ) (Open Access)We give an update o...
Hot subdwarf stars are evolved, subluminous, helium-burning stars, most likely formed when red-giant...
Hot subdwarfs (sdO/Bs) are the helium-burning cores of red giants, which have lost almost all of the...
We give an update of the results of a campaign to obtain orbital solutions of subdwarf B stars from ...