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Spectrophotometry of the Orion Nebula

Name: Spectrophotometry of the Orion Nebula
Creator: Janet P. Simpson
Keywords: 13. Climate action, 0103 physical sciences, 01 natural sciences

descriptionPublicationkeyboard_double_arrow_right Article 01 Oct 1973Publisher:IOP PublishingJournal:Publications of the Astronomical Society of the Pacific, volume 85, page 479 (issn: 0004-6280, eissn: 1538-3873,

Authors: Janet P. Simpson;

doi: 10.1086/129493

Spectrophotometry of the Orion Nebula

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Abstract

Observations of line and continuum strengths were made in six regions in the Orion nebula. From the observations, electron temperatures, electron densities, and chemical abundances are derived. A model for the Orion nebula is computed that agrees with the optical and radio observations of the nebula. Scattering and absorption by dust were added to the model and the predicted scattered continuum is compared to the observed continuum. Key words: H ii regions - Orion nebula - interstellar dust

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