SPECTROPHOTOMETRY OF GALACTIC NEBULAE ORION NEBULA III.
Abstract
The internal physical structure of the Orion Nebula has been investigated. A realistic model of the nebula has been developed, which deviates strongly from a symmetrically spherical model. The Trapezium stars are situated on one side of the radiating masses of the center, on the side to the observer. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Nov 30, 1964
- Accession Number
- AD0620117
Entities
People
- K. Wurm