The magnesium method for determining the electron density in stellar atmospheres

Details The magnesium method for determining the electron density in stellar atmospheres The magnesium method for determining the electron density in stellar atmospheres

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..458c&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, June 1985, p. 458-462) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, May-June

Astronomy and Astrophysics

Astronomy

1

A Stars, Electron Density (Concentration), Magnesium, Stellar Atmospheres, Ultraviolet Spectra, Spaceborne Astronomy, Spectrum Analysis, Stellar Spectrophotometry

Scientific paper

A method for determining the electron density in stellar atmospheres by using the ultraviolet resonance lines of neutral and ionized magnesium, 2852-A Mg I and 2795-A Mg II, is briefly described. The mean electron densities in the atmospheres of 31 type A0-G5 stars as well as the sun, which have been determined by using equivalent widths of the 2852-A and 2795-A lines recorded in experiments on the Orion 2, IUE, and other spacecraft, are presented.

Affiliated with

Also associated with

No associations

Rating

The magnesium method for determining the electron density 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 The magnesium method for determining the electron density in stellar atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The magnesium method for determining the electron density in stellar atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1669593