LTE line blanketing of an early B star atmosphere by ultraviolet lines using accurate damping constants

Details LTE line blanketing of an early B star atmosphere by ultraviolet lines using accurate damping constants LTE line blanketing of an early B star atmosphere by ultraviolet lines using accurate damping constants

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.181..777p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 181, Dec. 1977, p. 777-788.

Astronomy and Astrophysics

Astronomy

4

Atmospheric Models, B Stars, Early Stars, Line Spectra, Stellar Atmospheres, Ultraviolet Spectra, Elastic Damping, Fine Structure, H Lines, Metal Ions, Opacity, Surface Cooling, Temperature Distribution, Thermodynamic Equilibrium

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1977MNRAS.181..777P

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