New line profiles of sodium and potassium perturbed by helium for brown dwarf and very cool white dwarf stars

Details New line profiles of sodium and potassium perturbed by helium for brown dwarf and very cool white dwarf stars New line profiles of sodium and potassium perturbed by helium for brown dwarf and very cool white dwarf stars

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1058..308c&link_type=abstract

SPECTRAL LINE SHAPES: Volume 15-19th International Conference on Spectral Line Shapes. AIP Conference Proceedings, Volume 1058,

Physics

Low Luminosity Stars, Subdwarfs, And Brown Dwarfs, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Visible And Ultraviolet Spectra

Scientific paper

The optical spectra of L- and T-type dwarfs exhibit a continuum dominated by the far wings of the absorption profiles of the Na 3s-3p and K 4s-4p doublet perturbed by molecular hydrogen and helium. We report on our work on new calculations of line profiles of Na and K perturbed by He for the conditions prevailing in brown dwarf atmospheres and very cool white dwarfs.

Affiliated with

Also associated with

No associations

Rating

New line profiles of sodium and potassium perturbed by helium for brown dwarf and very cool white dwarf stars 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 New line profiles of sodium and potassium perturbed by helium for brown dwarf and very cool white dwarf stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New line profiles of sodium and potassium perturbed by helium for brown dwarf and very cool white dwarf stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1662827