Buscar
Mostrando ítems 41-50 de 539
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 ...
Radiation hydrodynamical turbulence in protoplanetary disks: Numerical models and observational constraints
(IOP Publishing Ltd, 2017)
Planets are born in protostellar disks, which are now observed with enough resolution to address questions about internal gas flows. Magnetic forces are possibly drivers of the flows, but ionization state estimates suggest ...
Increase of ionization fraction of dusty proto-stelLar accretion disks by damping of Alfvén waves
(International Astronomical UnionFlorianópolis, 2013)
The ambient of the cloud that gives rise to the process
of star formationconsisted of: turbulence, magnetic
field and dust. In general, in the process of
star formation there is the formation of an accretion
disk whose ...
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 ...