On the iron abundance in interstellar gas

Details On the iron abundance in interstellar gas On the iron abundance in interstellar gas

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....43..291o&link_type=abstract

Astronomy and Astrophysics, vol. 43, no. 2, Oct. 1975, p. 291-295.

Astronomy and Astrophysics

Astrophysics

22

Abundance, Collision Parameters, Electron Energy, Emission Spectra, Interstellar Gas, Iron, Electron States, Forbidden Transitions, Infrared Spectra, Ionization Cross Sections, Nebulae, Orion Constellation

Scientific paper

The iron abundance is determined in the Orion nebula from the observed
emission lines of Fe(+) and Fe(++). A comparison of the derived value
with the iron abundance in the sun and the interstellar medium is made.

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