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Modeling the Violet Spectral Region of Cool Stars: Line and Continuous Opacity
 

Summary: Modeling the Violet Spectral Region of Cool Stars: Line and
Continuous Opacity
C. Ian Short
Armagh Observatory
Armagh, Northern Ireland BT61 9DG
I: cis@star.arm.ac.uk
and
John B. Lester
Astronomy Department, Erindale College, University of Toronto
Mississauga, ON, Canada L5L 1C6
I: lester@astro.utoronto.ca
Received ; accepted

-- 2 --
ABSTRACT
The calculated flux distribution in the 300 to 400 nm region only fits the
observed distribution closely for both the Sun and Arcturus when the complete
atlas9 line list is used. However, a good fit to the detailed shape of the
observed high resolution spectrum in the Sun may only be obtained by using a
sub­set of this line list that only includes lines with the highest quality atomic

  

Source: Armagh Observatory

 

Collections: Physics