activity
20122026
most citedResolving the kinematics of the disks around Galactic B[e] supergiants

41 citations · 123 across the 17 of their papers we have counts for

collaborators
Showing 2022Show all

5 papers · 1 filter

astro-ph.SR2022★ 20 cited

Evolution of massive stars with new hydrodynamic wind models

A. C. Gormaz-Matamala, M. Curé, G. Meynet +3

Here we present evolutionary models for a set of massive stars, introducing a new prescription for the mass-loss rate obtained from hydrodynamical calculations in which the wind ve…

astro-ph.SR2022

Revisiting Viscous Transonic Decretion Disks of Be Stars

Michel Curé, Rodrigo Meneses, Ignacio Araya +4

In the context of Be stars, we restudied the viscous transonic decretion disk model of these stars. This model is driven by a radiative force due to an ensemble of optically-thin l…

astro-ph.SR2022

Application limit of the photocentre displacement to fundamental stellar parameters of fast rotators -- Illustration on the edge-on fast rotator Regulus

M. Hadjara, R. G. Petrov, S. Jankov +16

Differential Interferometry allows to obtain the differential visibility and phase, in addition to the spectrum. The differential phase contains important information about the str…

astro-ph.SR2022★ 12 cited

New self-consistent wind parameters fitting optical spectra of O-type stars observed with HERMES spectrograph

Alex C. Gormaz-Matamala, Michel Curé, Alex Lobel +5

We perform spectral fitting for a set of O-type stars based on self-consistent wind solutions, which provide mass-loss rate and velocity profiles directly derived from the initial…

astro-ph.SR2022★ 7 cited

Automatic algorithm to obtain values via Fourier Transform in BeSOS database

Martín Solar, Catalina Arcos, Michel Curé +2

Be stars are found to rotate close to their critical rotation and therefore they are considered as an important laboratory of study for stellar rotation. In this context, we obtain…