Highly Excited Hydrogen Lines in Stellar Spectra. I

Details Highly Excited Hydrogen Lines in Stellar Spectra. I Highly Excited Hydrogen Lines in Stellar Spectra. I

Sep 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..13...36b&link_type=abstract

Astrophysics and Space Science, Volume 13, Issue 1, pp.36-47

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

The solution of the hydrogenic Schrödinger equation are given with two boundary conditions imposed on the wave function, for distances of the order of magnitude of one hundred times the Bohr radius from the central nucleus. Thus the shifts and splitting of the Hγ-H26 lines are given which arise from the non-vacant environment. The Inglis-Teller limit is revised since from the shifts it follows that it gives a correct charged particle density only in the case of extremely high electron and ion densities. The gas density is derived from the number of the visible Balmer lines, and usually the widths and the contours but not the coalescence include information on the charged particle density.

Affiliated with

Also associated with

No associations

Rating

Highly Excited Hydrogen Lines in Stellar Spectra. I 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 Highly Excited Hydrogen Lines in Stellar Spectra. I, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Highly Excited Hydrogen Lines in Stellar Spectra. I will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1376689