Theoretical He I line intensities in low-density plasmas

Details Theoretical He I line intensities in low-density plasmas Theoretical He I line intensities in low-density plasmas

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.251..316s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 251, July 15, 1991, p. 316, 317.

Astronomy and Astrophysics

Astronomy

41

Astronomical Models, Helium, Line Spectra, Nebulae, Plasma Density, Plasma Spectra, Electron Density (Concentration), Infrared Spectroscopy

Scientific paper

The recombination spectra of He I in nebular conditions can be calculated by means of a capture-collision-cascade model based on Brocklehurst's (1972) method when the calculations of the 2(3)P-2(3)S series are corrected. Results are discussed for calculations which include temperatures from 312.5-20,000 K and electron densities of up to 10 to the 6th/cu cm. Line emissions from He I in the optical and IR bands can be interpreted by means of the calculations of recombination spectra.

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