Computations of NLTE Model Atmospheres and Synthetic Spectra at Université de Montréal: Applications to sdB Stars and AM CVn Systems

Details Computations of NLTE Model Atmospheres and Synthetic Spectra at Université de Montréal: Applications to sdB Stars and AM CVn Systems Computations of NLTE Model Atmospheres and Synthetic Spectra at Université de Montréal: Applications to sdB Stars and AM CVn Systems

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273..259b&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 259-262 (2010).

Physics

2

Dwarf Stars, Accretion Disks, Spectral Analysis, Interstellar Matter, Main-Sequence: Late-Type Stars, Accretion And Accretion Disks, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Physical Properties

Scientific paper

We briefly present here our first results of our ongoing efforts to
produce large grids of NLTE synthetic spectra for hot subdwarf stars and
pure helium accretion disks.

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