Disks around Young Brown Dwarfs
First Author:
Lucia Adame
Email: adamel AT astroscu.unam.mx
Instituto de Astronomia, UNAM
Apartado Postal 70 - 264, Ciudad Universitaria
Mexico, D.F., CP 04510, Mexico
Coauthors:
D'Alessio, Paola, Centro de Radioastronomia y Astrofisica, UNAM
Calvet, Nuria, University of Michigan
Abstract
We modify the computational codes developed by D'Alessio and colaborators to obtain the IRAC synthetic colors for young brown dwarfs with disks in Taurus. A set of models, ranging several mass accretion rates, substellar effective temperature, and alpha-viscosity parameter, are constructed; with that, and using previously published IRAC data, we study the innermost region of the circunsubstellar accretion disks in the Taurus region. The median SED of Taurus for stellar/substellar objects with spectral types between M6 and M9 is obtained.
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