CCD-BASED SPECTROSCOPY OF WOLF-RAYET STARS: STUDY OF EXPANSION VELOCITY AND MASS LOSS AS A CONTRIBUTOR IN INTERSTELLAR MATTER ENRICHMENT
Wolf-Rayet stars was discovered by C.Wolf and G.Rayet in 1867. In the spectra of Wolf-Rayet stars, broad emission lines caused by Doppler broadening can be observed. This indicate that Wolf-Rayet stars have high expansion velocity. It is also known that Wolf-Rayet stars have high mass loss rates com...
Saved in:
主要作者: | |
---|---|
格式: | Final Project |
語言: | Indonesia |
在線閱讀: | https://digilib.itb.ac.id/gdl/view/36136 |
標簽: |
添加標簽
沒有標簽, 成為第一個標記此記錄!
|