Spatial heterodyne interferometry of VY Canis Majoris, alpha Orionis, alpha Scorpii, and R Leonis at 11 microns
Technical Report
·
OSTI ID:5301597
Using the technique of heterodyne interferometry, measurements were made of the spatial distribution of 11 micron radiation from four late type stars. The circumstellar shells surrounding VY Canis Majoris, alpha Orionis, and alpha Scorpii were resolved, whereas that of R Leonis was only partially resolved at a fringe spacing of 0.4 sec.
- Research Organization:
- California Univ., Berkeley (USA). Dept. of Physics
- OSTI ID:
- 5301597
- Report Number(s):
- N-77-27049
- Country of Publication:
- United States
- Language:
- English
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