Relationship between the line and continuum emission of hydrogen plasma

Details Relationship between the line and continuum emission of hydrogen plasma Relationship between the line and continuum emission of hydrogen plasma

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..924k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Sept.-Oct. 1990, p. 924-934. In Russian.

Astronomy and Astrophysics

Astronomy

5

Balmer Series, Continuous Radiation, Hydrogen Plasma, Line Spectra, Plasma Radiation, Stellar Spectra, Gas Ionization, Plasma Spectra

Scientific paper

Calculations of the line and continuum emission of hydrogen plasma are performed for a wide range of electron temperature and density on the basis of Sobolev's escape-probabiluity method for the case of the collisional excitations and ionizations of hydrogen atoms. The relative intensities of the Balmer series lines are calculated for electron temperatures ranging from 10,000 to 25,000 K and for electron densities ranging from 10 to the 9th to 10 to the 14th/cu cm. The calculations are applied to T Tauri and UV Ceti type stars.

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