The ratio of optical to near-infrared emission line strengths in S II as electron density diagnostics for planetary nebulae

Details The ratio of optical to near-infrared emission line strengths in S II as electron density diagnostics for planetary nebulae The ratio of optical to near-infrared emission line strengths in S II as electron density diagnostics for planetary nebulae

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.186..277k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 186, no. 2, Dec. 1991, p. 277-281.

Astronomy and Astrophysics

Astrophysics

1

Electron Density (Concentration), Emission Spectra, Near Infrared Radiation, Planetary Nebulae, Atomic Energy Levels, Electron Energy, Ionization Potentials

Scientific paper

Einstein A-coefficients for transitions in S ii, calculated with the
atomic structure package CIV3, are used to derive the electron density
sensitive emission line rati

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