Near-infrared Fourier spectroscopy of the Orion Nebula

Details Near-infrared Fourier spectroscopy of the Orion Nebula Near-infrared Fourier spectroscopy of the Orion Nebula

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...214..712l&link_type=abstract

Astrophysical Journal, Part 1, vol. 214, June 15, 1977, p. 712-717. Research supported by the National Research Council of Cana

Astronomy and Astrophysics

Astrophysics

11

Fourier Analysis, Infrared Spectroscopy, Michelson Interferometers, Near Infrared Radiation, Nebulae, Stellar Spectrophotometry, Astronomical Models, Emission Spectra, Line Spectra, Signal To Noise Ratios

Scientific paper

Observations of two regions of the Orion Nebula from 9000 to 16,000 A have been made with a dynamic Michelson interferometer. Relative intensities and surface brightness for emission lines in this region are given. Observation of the 13,165-A multiplet of O I supports the direct starlight excitation mechanism as modeled by Grandi (1975) to explain the permitted line emission.

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