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Application of a local-spectrum correlated model to modeling radiative transfer in a mixture of real gas media in bidimensional enclosures
(Taylor & Francis IncPhiladelphiaEUA, 2005)
Consistent dust and gas models for protoplanetary disks I. Disk shape, dust settling, opacities, and PAHs
(EDP SCIENCES, 2016)
We propose a set of standard assumptions for the modelling of Class II and III protoplanetary disks, which includes detailed continuum radiative transfer, thermo-chemical modelling of gas and ice, and line radiative transfer ...
Obtenção dos coeficientes de absorção a partir dos parâmetros de linha contidos no banco de dados HITEMP 2010
(Universidade Federal do Rio Grande do NorteBrasilUFRNEngenharia Mecânica, 2018-12-11)
The objective of this work was to obtain the absorption coefficients of H2O at different temperatures from 500 K to 2500 K, varying by 50 K, from the line parameters contained in the HITEMP 2010 database. The JavaHawks ...
Supernovae from massive stars with extended tenuous envelopes
(EDP Sciences S A, 2018)
Massive stars with a core-halo structure are interesting objects for stellar physics and hydrodynamics. Using simulations for stellar evolution, radiation hydrodynamics, and radiative transfer, we study the explosion of ...
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 ...