Symposium on the Orion Nebula to Honor Henry Draper, New York University, New York, NY, December 4, 5, 1981, Proceedings

Astronomy and Astrophysics – Astronomy

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Conferences, Orion Nebula, Stellar Evolution, Astronomical Models, B Stars, Carbon Monoxide, Hydrogen Clouds, Interstellar Matter, Line Spectra, Masers, Molecular Clouds, O Stars, Radio Sources (Astronomy), Star Distribution, Stellar Envelopes

Scientific paper

The present conference on astronomical studies of the Orion Nebula covers molecular clouds in Orion, the use of the nebula's cloak as a model for gas super-shells around OB associations, optical and UV data concerning the nebula's physical conditions, the presence of atomic carbon in Orion, large scale distribution of far-IR and sub-mm line emission, star formation studies in the IR, gas dynamics in the circumstellar nebula of the Becklin-Neugebauer source, maser sources and far-IR CO line emission in Orion-KL, and synthesis maps of mm molecular lines. Also discussed are Orion's star distributions, core region nebular condensations, energetic molecular flows in star-forming cloud cores, IR observations of HH objects, compact continuum radio sources, the SiO maser, shock waves, and the chemical evolution of OB associations. For individual items see A83-39700 to A83-39730

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