The Morphology and Uniformity of Circumstellar OH/H<sub>2</sub>O Masers around OH/IR Stars
Even though low mass stars (< 8 solar masses) vastly outnumber high mass stars (< 8 solar masses), the more massive stars drive the chemical evolution of galaxies from which the next generation of stars and planets can form. Understanding mass loss of asymptotic giant branch stars contributes...
| Main Author: | |
|---|---|
| Format: | Others |
| Published: |
BYU ScholarsArchive
2017
|
| Subjects: | |
| Online Access: | https://scholarsarchive.byu.edu/etd/6633 https://scholarsarchive.byu.edu/cgi/viewcontent.cgi?article=7633&context=etd |