activity
20122017
most citedThe orbits of subdwarf-B + main-sequence binaries: III. The period - eccentricity distribution

68 citations · 266 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2017

Constraining Roche-Lobe Overflow Models Using the Hot-Subdwarf Wide Binary Population

Joris Vos, Maja Vučković

One of the important issues regarding the final evolution of stars is the impact of binarity. A rich zoo of peculiar, evolved objects are born from the interaction between the loos…

astro-ph.SR201710 cited

Evolutionary Constraints on the Long-period Subdwarf B Binary PG 1018-047

J. Deca, J. Vos, P. Németh +4

We have revisited the sdB+K-star long-period binary PG 1018-047 based on 20 new high-resolution VLT/UVES spectra that provided regular coverage over a period of more than 26 months…

astro-ph.SR201757 cited

Composite hot-subdwarf binaries -- I. The spectroscopically confirmed sdB sample

Joris Vos, Péter Németh, Maja Vučković +2

Hot subdwarf-B (sdB) stars in long-period binaries are found to be on eccentric orbits, even though current binary-evolution theory predicts these objects to be circularised before…

astro-ph.SR201768 cited

The orbits of subdwarf-B + main-sequence binaries: III. The period - eccentricity distribution

Joris Vos, Roy H. Østensen, Maja Vuckovic +1

The predicted orbital-period distribution of the subdwarf-B (sdB) population is bi-modal with a peak at short (< 10 days) and long (> 500 days) periods. Observationally, many short…

astro-ph.SR201566 cited

Testing eccentricity pumping mechanisms to model eccentric long period sdB binaries with MESA

Joris Vos, Roy Østensen, Pablo Marchant +1

Hot subdwarf-B stars in long-period binaries are found to be on eccentric orbits, even though current binary-evolution theory predicts those objects to be circularised before the o…

astro-ph.SR201265 cited

The orbits of subdwarf B + main-sequence binaries. I: The sdB+G0 system PG 1104+243

J. Vos, R. H. Östensen, P. Degroote +18

The predicted orbital period histogram of an sdB population is bimodal with a peak at short (< 10 days) and long (> 250 days) periods. Observationally, there are many short-period…