O
Onno R. Pols
Researcher at Radboud University Nijmegen
Publications - 126
Citations - 9072
Onno R. Pols is an academic researcher from Radboud University Nijmegen. The author has contributed to research in topics: Stars & Stellar evolution. The author has an hindex of 39, co-authored 124 publications receiving 8008 citations. Previous affiliations of Onno R. Pols include Spanish National Research Council & Utrecht University.
Papers
More filters
Journal ArticleDOI
Evolution of binary stars and the effect of tides on binary populations
TL;DR: In this paper, a rapid binary-evolution algorithm was proposed to model the formation and evolution of binary systems, including all aspects of single-star evolution, features such as mass transfer, mass accretion, common envelope evolution, collisions, supernova kicks and angular momentum loss mechanisms.
Journal ArticleDOI
Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
TL;DR: In this article, the authors present analytic formulae that approximate the evolution of stars for a wide range of mass M and metallicity Z, including all phases from the zero-age main sequence up to, and including, the remnant stages.
Journal ArticleDOI
Massive binaries as the source of abundance anomalies in globular clusters
TL;DR: In this paper, the authors compute the evolution of a 20 M star in a close binary considering the effects of non-conservative mass and angular momentum transfer and of rotation and tidal interaction to demonstrate the principle.
Journal ArticleDOI
A new synthetic model for asymptotic giant branch stars
TL;DR: In this article, a synthetic model for thermally pulsing asymptotic giant branch (TPAGB) evolution constructed by fitting expressions to full evolutionary models in the metallicity range 0.0001 Z 0.02 was presented.
Journal ArticleDOI
Rotational mixing in massive binaries - Detached short-period systems
S. E. de Mink,Matteo Cantiello,Norbert Langer,Norbert Langer,Onno R. Pols,Ines Brott,S.-Ch. Yoon +6 more
TL;DR: In this article, the effects of rotational mixing on the surface enhancements of massive main-sequence stars in short-period binary systems were investigated using a state-of-the-art stellar evolution code including the effect of rotation, tides, and magnetic fields.