Levenhagen 2017

A grid of LTE and non-LTE synthetic spectra of hot DA white dwarfs. It covers Teff from 17,000 K to 100,000 K and log(g) from 7.0 to 9.5. The stellar models are built for pure hydrogen and the spectra cover a wavelength range from 90 nm to 2.5 micron.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/svo.cab/models/levenhagen
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/levenhagen
Provenance
Creator Levenhagen, Diaz, Coelho, Hubeny, ApJ Volume 231, Issue 1, article id. 1, 6 pp. (2017).
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