BT-DUSTY

The BT-DUSTY Model grid of theoretical spectra. Brown dwarfs/extrasolar planets atmosphere models without irradiation but including dust opacity (fully efficient dust settling) and updated abundances. Wavelengths have been converted to air wavelengths.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/svo.cab/models/bt-dusty
Related Identifier http://svo.cab.inta-csic.es/
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://svo.cab/models/bt-dusty
Provenance
Creator Hauschildt, P.H., Allard, F., Baron, E., ApJ 512, 377, 1999
Publisher SVO CAB
Publication Year 2010
OpenAccess true
Contact Enrique Solano, LAEFF Archive Support Team <esm(at)cab.inta-csic.es>
Representation
Resource Type Other; AstroObjects
Version 1.0
Discipline Astrophysics and Astronomy