448 citations · 477 across the 7 of their papers we have counts for
9 papers
Turbulent viscosity in line-driven stellar winds
Matías Montesinos, Michel Cure, Ignacio Araya +1
Radiation-driven winds from massive stars generate powerful outflows known to be intrinsically turbulent. Despite this, standard hydrodynamic models have historically restricted th…
Quasi-Keplerian Be-Star Disks with Mimicking Viscosity
Michel Cure, Ignacio Araya, Rodrigo Meneses +5
Classical Be stars are fast-rotating B-type stars with gaseous quasi-Keplerian disks formed by equatorial ejection of material. While the viscous decretion disk (VDD) model reprodu…
New self-consistent theoretical descriptions for mass-loss rates of O-type stars
F. Figueroa-Tapia, J. A. Panei, M. Curé +5
Massive O-type stars lose a significant fraction of their mass through radiation-driven winds, a process that critically shapes their evolution and feedback into the interstellar m…
ISOSCELES project: A grid-based quantitative spectroscopic analysis of massive stars
I. Araya, M. Curé, N. Machuca +4
Massive stars play a fundamental role in galactic evolution through their strong stellar winds, chemical enrichment, and feedback mechanisms. Accurate modelling of their atmosphere…
Analytical Solutions for Radiation-Driven Winds in Massive Stars II: The -slow Regime
I. Araya, A. Christen, M. Curé +7
Accurate mass-loss rates and terminal velocities from massive stars winds are essential to obtain synthetic spectra from radiative transfer calculations and to determine the evolut…
Self-consistent solutions for line-driven winds of hot massive stars. The m-CAK procedure
Alex C. Gormaz-Matamala, Michel Curé, Lydia S. Cidale +1
Massive stars present strong stellar that which are described by the radiation driven wind theory. Accurate mass-loss rates are necessary to properly describe the stellar evolution…
Wind properties of variable B supergiants. Evidence of pulsations connected with mass-loss episodes
M. Haucke, L. S. Cidale, R. O. J. Venero +4
Variable B supergiants (BSGs) constitute a heterogeneous group of stars with complex photometric and spectroscopic behaviours. They exhibit mass-loss variations and experience diff…
Pulsations as a mass-loss trigger in evolved hot stars
Michaela Kraus, Dieter H. Nickeler, Maximiliano Haucke +5
During the post-main sequence evolution massive stars pass through several short-lived phases, in which they experience enhanced mass loss in the form of clumped winds and mass eje…
Atmospheric NLTE-Models for the Spectroscopic Analysis of Blue Stars with Winds. II. Line-Blanketed Models
J. Puls, M. A. Urbaneja, R. Venero +4
We present new or improved methods for calculating NLTE, line-blanketed model atmospheres for hot stars with winds (spectral types A to O), with particular emphasis on a fast perfo…