INVESTIGATION OF ACCRETION DISK INSTABILITY IN BLACK HOLE X-RAY TRANSIENT THROUGH ANALYSIS OF THE X-RAY LIGHT CURVE AND SPECTRAL VARIABILITY
One of the Black Hole X-ray Transient (BHXT) with the largest black hole mass and longest orbital period in the Galaxy, GRS 1915+105, has been active for 26 years since its discovery in 1992 and has been observed several times in the super-Eddington state before entering quiescent in 2018. Aside...
Saved in:
| 主要作者: | |
|---|---|
| 格式: | Theses |
| 語言: | Indonesia |
| 在線閱讀: | https://digilib.itb.ac.id/gdl/view/86914 |
| 標簽: |
添加標簽
沒有標簽, 成為第一個標記此記錄!
|