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Evolution of rotating massive stars with new hydrodynamic wind models
A. C. Gormaz-Matamala
,
J. Cuadra
, G. Meynet
, M. Curé
Faculty of Liberal Arts
Research output
:
Contribution to journal
›
Article
›
peer-review
15
Scopus citations
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Keyphrases
26Al
16%
Additional Term
16%
Angular Momentum
16%
Correction Factor
16%
Evolution Model
33%
Evolutionary
33%
Evolutionary Model
16%
Force Line
16%
Force Parameters
16%
Galactic
33%
Galactic Center
16%
Helium
16%
High Brightness
16%
Interstellar Medium
16%
K Parameter
16%
Large Magellanic Cloud
16%
Low-mass
16%
Main Sequence
33%
Mass Loss
50%
Mass Loss Rate
50%
Massive Models
16%
Massive Stars
100%
Metallicity
33%
Mixing Efficiency
16%
Multiple Systems
16%
O-type
16%
Research-based
16%
Rotational Velocity
16%
Self-consistent Approach
16%
Self-consistent Model
16%
Simultaneous Calculations
16%
Single System
16%
Stellar Evolution
16%
Stellar Rotation
33%
Stellar Structure
16%
Stellar Winds
16%
Weak Winds
50%
Wind Model
100%
INIS
abundance
14%
acceleration
14%
aluminium 26
14%
angular momentum
14%
corrections
14%
grids
28%
helium
14%
hydrodynamics
100%
isotopes
14%
luminosity
14%
magellanic clouds
14%
mass loss
85%
metallicity
28%
mixing
14%
populations
14%
range
28%
reduction
14%
rotation
57%
solutions
14%
star evolution
14%
stars
14%
stellar winds
14%
surfaces
14%
surveys
14%
tracks
57%
values
28%
velocity
14%
wind
100%
Physics
Angular Momentum
16%
Galactic Center
16%
Interstellar Matter
16%
Large Magellanic Cloud
16%
Massive Star
100%
Metallicity
33%
Stellar Evolution
16%
Stellar Rotation
33%
Stellar Structure
16%
Stellar Wind
16%