Temperature and density determination from SI III lines

Details Temperature and density determination from SI III lines Temperature and density determination from SI III lines

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...155..205n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 155, no. 1, Jan. 1986, p. 205-209.

Astronomy and Astrophysics

Astrophysics

41

Gas Density, Gas Temperature, Line Spectra, Planetary Nebulae, Silicon, Atomic Spectra, Emissivity, Oscillator Strengths, Symbiotic Stars, Transition Probabilities

Scientific paper

It is shown how under conditions of gaseous nebulae, the temperature
Te and the density Ne can be derived from observed
Si III fluxes at λλ 1206.5, 1301, 1882.7, 1892.0.
Transition probabilities among the energetically 17 lowest terms are
given and theoretical line intensity ratios are calculated.

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