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...
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| المؤلف الرئيسي: | |
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| التنسيق: | Theses |
| اللغة: | Indonesia |
| الوصول للمادة أونلاين: | https://digilib.itb.ac.id/gdl/view/86914 |
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