activity
19992021
most citedEmission lines from rotating proto-stellar jets with variable velocity profiles. I. Three-dimensional numerical simulation of the non-magnetic case

49 citations · 136 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2021

Monte-Carlo simulations of evolving rotational distributions of low-mass stars in young open clusters. Testing the influence of initial conditions

Maria Jaqueline Vasconcelos, Jérôme Bouvier, Florian Gallet +1

The rotational evolution of a young stellar population can give informations about the rotation pattern of more evolved clusters. Combined with rotational period values of thousand…

astro-ph.SR2016★ 7 cited

Investigating the rotational evolution of very low-mass stars and brown dwarfs in young clusters using Monte Carlo simulations

M. J. Vasconcelos, J. Bouvier

Context. Very low-mass (VLM) stars and brown dwarfs (BDs) present a different rotational behaviour from their solar mass counter-parts. Aims. We investigate the rotational evolutio…

astro-ph.SR2015★ 5 cited

Principal Component Analysis of computed emission lines from proto-stellar jets

A. H. Cerqueira, J. Reyes-Iturbide, F. De Colle +1

A very important issue concerning protostellar jets is the mechanism behind their formation. Obtaining information on the region at the base of a jet can shed light into the subjec…

astro-ph.SR2015★ 21 cited

Investigating the rotational evolution of young, low mass stars using Monte Carlo simulations

M. J. Vasconcelos, J. Bouvier

We investigate the rotational evolution of young stars through Monte Carlo simulations. We simulate 280,000 stars, each of which is assigned a mass, a rotational period, and a mass…

astro-ph.SR2015★ 3 cited

Gemini-IFU spectroscopy of HH 111

A. H. Cerqueira, M. J. Vasconcelos, A. C. Raga +2

We present new optical observations of the HH 111 Herbig-Haro jet using the Gemini Multi Object Spectrograph in its Integral Field Unit mode. Eight fields of 5" x 3.5" have been po…

astro-ph.SR2013

The photoevaporation of a neutral structure by an EUV+FUV radiation field

V. Lora, M. J. Vasconcelos, A. C. Raga +2

The EUV photoionizing radiation and FUV dissociating radiation from newly born stars photoevaporate their parental neutral cloud, leading to the formation of dense clumps that coul…