OPAL opacities for astrophysical applications

Details OPAL opacities for astrophysical applications OPAL opacities for astrophysical applications

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991rphd.work...22i&link_type=abstract

Presented at the International Workshop on Radiative Properties of Hot Dense Matter, Sarasota, FL, 22-26 Oct. 1990

Astronomy and Astrophysics

Astrophysics

Astrophysics, Atomic Structure, Computer Programs, Equations Of State, Opacity, Solar Neutrinos, Computers, Lithium, Solar Radiation

Scientific paper

The OPAL opacity code developed at LLNL has been applied to astrophysical problems. The computed Rosseland mean opacities show significant differences when compared to the Los Alamos results. These differences have been traced to both atomic and equation of state improvements in the OPAL code. Furthermore, preliminary work suggest that the OPAL calculations considerably improve the agreement between observations and stellar models.

Affiliated with

Also associated with

No associations

Rating

OPAL opacities for astrophysical applications does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with OPAL opacities for astrophysical applications, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and OPAL opacities for astrophysical applications will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1040482