Contains fulltext : 84424.pdf (publisher's version ) (Closed access
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...
Neutron stars and stellar-mass black holes are the remnants of massive stars, which ended their live...
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...
Contains fulltext : 143841.pdf (preprint version ) (Open Access
Contains fulltext : 94131.pdf (preprint version ) (Open Access)Fifth Meeting on Ho...
HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this gro...
A large fraction of the sdB stars reside in short period binaries. It is therefore clear that binary...
Context. Hot subdwarfs are core-helium burning stars that show lower masses and higher temperatures ...
About a third of the hot subdwarfs of spectral type B, which are mostly core-helium burning objects ...
Hot subdwarf stars are evolved, subluminous, helium-burning stars, most likely formed when red-giant...
Massive stars are born in close binaries, and in the course of their evolution, the initially more m...
Contains fulltext : 94006.pdf (preprint version ) (Open Access
Contains fulltext : 159658.pdf (preprint version ) (Open Access
Contains fulltext : 157958.pdf (preprint version ) (Open Access)New spectroscopic ...
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 ...
Neutron stars and stellar-mass black holes are the remnants of massive stars, which ended their live...
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...
Contains fulltext : 143841.pdf (preprint version ) (Open Access
Contains fulltext : 94131.pdf (preprint version ) (Open Access)Fifth Meeting on Ho...
HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this gro...
A large fraction of the sdB stars reside in short period binaries. It is therefore clear that binary...
Context. Hot subdwarfs are core-helium burning stars that show lower masses and higher temperatures ...
About a third of the hot subdwarfs of spectral type B, which are mostly core-helium burning objects ...
Hot subdwarf stars are evolved, subluminous, helium-burning stars, most likely formed when red-giant...
Massive stars are born in close binaries, and in the course of their evolution, the initially more m...
Contains fulltext : 94006.pdf (preprint version ) (Open Access
Contains fulltext : 159658.pdf (preprint version ) (Open Access
Contains fulltext : 157958.pdf (preprint version ) (Open Access)New spectroscopic ...
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 ...
Neutron stars and stellar-mass black holes are the remnants of massive stars, which ended their live...
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at ...