63 citations · 213 across the 5 of their papers we have counts for
9 papers
Grids of stellar models with rotation: V. Models from 1.7 to 120 Msun at zero metallicity
Laura J. Murphy, Jose H. Groh, Sylvia Ekstrom +10
Understanding the nature of the first stars is key to understanding the early universe. With new facilities such as JWST we may soon have the first observations of the earliest ste…
On the ALMA observability of nascent massive multiple systems formed by gravitational instability
D. M. -A. Meyer, A. Kreplin, S. Kraus +3
Massive young stellar object (MYSOs) form during the collapse of high-mass pre-stellar cores, where infalling molecular material is accreted through a centrifugally-balanced accret…
Stellar models and isochrones from low-mass to massive stars including pre-main sequence phase with accretion
L. Haemmerlé, P. Eggenberger, S. Ekström +6
Grids of stellar models are useful tools to derive the properties of stellar clusters, in particular young clusters hosting massive stars, and to provide information on the star fo…
On the episodic excursions of massive protostars in the Hertzsprung-Russell diagram
D. M. A. Meyer, L. Haemmerlé, E. I. Vorobyov
Massive protostars grow and evolve under the effect of rapid accretion of circumstellar gas and dust, falling at high rates (-).…
Formation of massive black holes via collisions and accretion
D. R. G. Schleicher, M. A. Fellhauer, T. Boekholt +13
To explain the observed population of supermassive black holes at z~7, very massive seed black holes or, alternatively, super-Eddington scenarios are needed to reach final masses o…
The magnetic fields of intermediate-mass T Tauri stars : I. Magnetic detections and fundamental stellar parameters
Florent Villebrun, Evelyne Alecian, Gaitee Hussain +13
Context. The origin of the fossil magnetic fields detected in 5 to 10% of intermediate-mass main sequence stars is still highly debated. Aims. We want to bring observational constr…