Hydrogenic Line Widths Produced By Energy Fluctuations In Stellar Atmospheres

Details Hydrogenic Line Widths Produced By Energy Fluctuations In Stellar Atmospheres Hydrogenic Line Widths Produced By Energy Fluctuations In Stellar Atmospheres

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1171..349c&link_type=abstract

RECENT DIRECTIONS IN ASTROPHYSICAL QUANTITATIVE SPECTROSCOPY AND RADIATION HYDRODYNAMICS: Proceedings of the International Confe

Astronomy and Astrophysics

Astrophysics

1

Spectral Line Breadth, Stellar Atmospheres, Binary Stars, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Binary And Multiple Stars

Scientific paper

A new method for obtaining the widths of spectral lines generated by energy fluctuations is presented. The energy changes of the atomic states are equated with the fractional fluctuations in energy to yield a formula for the line widths. Comparing the formula for the line widths with some published experimental and theoretical values show good agreement.

Affiliated with

Also associated with

No associations

Rating

Hydrogenic Line Widths Produced By Energy Fluctuations In Stellar Atmospheres 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 Hydrogenic Line Widths Produced By Energy Fluctuations In Stellar Atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hydrogenic Line Widths Produced By Energy Fluctuations In Stellar Atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1272270