Emission from an Inhomogeneous Plasma: Line Intensities and Determination of Elemental Abundances in Gaseous Nebulae with Fluctuations of Te and ne

Details Emission from an Inhomogeneous Plasma: Line Intensities and Determination of Elemental Abundances in Gaseous Nebulae with Fluctuations of Te and ne Emission from an Inhomogeneous Plasma: Line Intensities and Determination of Elemental Abundances in Gaseous Nebulae with Fluctuations of Te and ne

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ap.....43..463k&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 43, Issue 4, p. 463-473 (2000).

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

A method is proposed for determining the abundances of chemical elements in planetary nebulae based on allowance for the actual distribution functions of errors in measuring line intensities. Fluctuations both in temperature and in mass density of a nebula are taken into account in the proposed method. The results of a determination of C and O abundances and of the amplitudes of temperature and density fluctuations are given.

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