most citedBONNSAI: a Bayesian tool for comparing stars with stellar evolution models

188 citations · 523 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201587 cited

The VLT-FLAMES Tarantula Survey XIX. B-type Supergiants - Atmospheric parameters and nitrogen abundances to investigate the role of binarity and the width of the main sequence

C. M. McEvoy, P. L. Dufton, C. J. Evans +19

TLUSTY non-LTE model atmosphere calculations have been used to determine atmospheric parameters and nitrogen (N) abundances for 34 single and 18 binary B-type supergiants (BSGs). T…

astro-ph.SR201459 cited

Orbital and physical properties of the Ori Aa,Ab,B triple system

Simón-Díaz, J. A. Caballero, J. Lorenzo +11

We provide a complete characterization of the astrophysical properties of the Ori Aa,Ab,B hierarchical triple system, and an improved set of orbital parameters for the highly e…

astro-ph.SR201428 cited

The occurrence of classical Cepheids in binary systems

Hilding R. Neilson, Fabian R. N. Schneider, Robert G. Izzard +2

Classical Cepheids, like binary stars, are laboratories for stellar evolution and Cepheids in binary systems are especially powerful ones. About one-third of Galactic Cepheids are…

astro-ph.SR2014153 cited

The spectroscopic Hertzsprung-Russell diagram of Galactic massive stars

N. Castro, L. Fossati, N. Langer +3

The distribution of stars in the Hertzsprung-Russell diagram narrates their evolutionary history and directly assesses their properties. Placing stars in this diagram however requi…

astro-ph.SR20148 cited

Numerical Tests of Rotational Mixing in Massive Stars with the new Population Synthesis Code BONNFIRES

Herbert H. B. Lau, Robert G. Izzard, Fabian R. N. Schneider

We use our new population synthesis code BONNFIRES to test how surface abundances predicted by rotating stellar models depend on the numerical treatment of rotational mixing, such…

astro-ph.SR2014188 cited

BONNSAI: a Bayesian tool for comparing stars with stellar evolution models

Fabian R. N. Schneider, Norbert Langer, Alex de Koter +3

Powerful telescopes equipped with multi-fibre or integral field spectrographs combined with detailed models of stellar atmospheres and automated fitting techniques allow for the an…