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Envolventes y discos protoplanetarios /
(2010-03)
En esta Tesis se presentan los resultados del modelado de diversos tipos de observaciones de dos grupos de estrellas en formación, con edades de aproximadamente 105 - 106 años. El primer grupo corresponde a las etapas de ...
The Gaia-ESO Survey: A new diagnostic for accretion and outflow activity in the young cluster NGC 2264
(European Southern Observatory, 2020)
Context. NGC 2264 is a young cluster whose accretion properties can be investigated in detail by taking advantage of the FLAMES data in the context of the Gaia-ESO Survey. In fact, the analysis of the Hα emission line ...
Erratum: Cooling in the shade of warped transition disks
(Oxford University Press, 2020)
This is an Erratum to the paper ‘Cooling in the shade of warped transition disks’ that was published in MNRAS, 486, L58-L62 (2019). The x-axis of Fig. 1 in the original version of the paper is incorrectly labeled, the ...
Investigating the magnetospheric accretion process in the young pre-transitional disk system DoAr 44 (V2062 Oph)
(European Southern Observatory, 2020)
Context. Young stars interact with their accretion disk through their strong magnetosphere.
Aims. We aim to investigate the magnetospheric accretion/ejection process in the young stellar system DoAr 44 (V2062 Oph).
Methods. ...
The eccentricity distribution of giant planets and their relation to super-Earths in the pebble accretion scenario
(2020-11-01)
Observations of the population of cold Jupiter planets (r >1 AU) show that nearly all of these planets orbit their host star on eccentric orbits. For planets up to a few Jupiter masses, eccentric orbits are thought to be ...
A METHOD FOR THE STUDY OF ACCRETION DISK EMISSION IN CATACLYSMIC VARIABLES. I. THE MODEL
(IOP PUBLISHING LTD, 2011)
We have developed a spectrum synthesis method for modeling the ultraviolet (UV) emission from the accretion disk from cataclysmic variables (CVs). The disk is separated into concentric rings, with an internal structure ...
FARGO3D: A new GPU-oriented MHD code
(IOP Publishing, 2016-03)
We present the FARGO3D code, recently publicly released. It is a magnetohydrodynamics code developed with special emphasis on the physics of protoplanetary disks and planet-disk interactions, and parallelized with MPI. The ...