500 citations
- Institute of AstronomyRU2 papers
- University of CambridgeGB2 papers
- American Institute of Aeronautics and AstronauticsUS1 paper
- Ames Research CenterUS1 paper
- CEA Paris-SaclayFR1 paper
- CEA Paris-Saclay - Etablissement de SaclayFR1 paper
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR1 paper
- Goddard Space Flight CenterUS1 paper
- Hokkaido UniversityJP1 paper
- Institut de Planétologie et d'Astrophysique de GrenobleFR1 paper
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR1 paper
- Leibniz Institute for Astrophysics PotsdamDE1 paper
11 papers
M&m's: An error budget and performance simulator code for polarimetric systems
Maria de Juan Ovelar, Frans Snik, Christoph U. Keller
Although different approaches to model a polarimeter's accuracy have been described before, a complete error budgeting tool for polarimetric systems has not been yet developed. Bas…
SPICES: Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems
Anthony Boccaletti, Jean Schneider, Wes Traub +28
SPICES (Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems) is a five-year M-class mission proposed to ESA Cosmic Vision. Its purpose is to image and charact…
GALEV evolutionary synthesis models - I. Code, input physics and web-interface
Ralf Kotulla, Uta Fritze, Peter Weilbacher +1
GALEV evolutionary synthesis models describe the evolution of stellar populations in general, of star clusters as well as of galaxies, both in terms of resolved stellar populations…
The evolution of runaway stellar collision products
E. Glebbeek, E. Gaburov, S. E. de Mink +2
In the cores of young dense star clusters repeated stellar collisions involving the same object can occur, which has been suggested to lead to the formation of an intermediate-mass…
Modelling the evolution and nucleosynthesis of carbon-enhanced metal-poor stars
O. R. Pols, R. G. Izzard, M. Lugaro +1
We present the results of binary population simulations of carbon-enhanced metal-poor (CEMP) stars. We show that nitrogen and fluorine are useful tracers of the origin of CEMP star…
Thermohaline mixing and gravitational settling in carbon-enhanced metal-poor stars
Richard J. Stancliffe, Evert Glebbeek
We investigate the formation of carbon-enhanced metal-poor (CEMP) stars via the scenario of mass transfer from a carbon-rich asymptotic giant branch (AGB) primary to a low-mass com…