| Autor: |
G. Chin, Frank J. Lovas, D. Glenar, M. J. Mumma, David Buhl, F. O. Clark, T. Kostiuk |
| Rok vydání: |
1980 |
| Předmět: |
|
| Zdroj: |
Symposium - International Astronomical Union. 87:537-538 |
| ISSN: |
0074-1809 |
| Popis: |
Published data on a select group of SiO maser sources have been analyzed for velocity variations as a function of phase. No apparent correlation was found to a level of about 2 km/s. This places constraints on the location of the maser molecules. Such a correlation should be present at some level. The implications for future high resolution infrared measurements are discussed. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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