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| 041 |
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|a eng
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| 100 |
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|9 568966
|a Siddiqi, Maham
|e Author
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| 245 |
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|a Fourier Resolved Spectroscopy of X-Ray Binary Stars
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| 260 |
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|a مسقط
|c 2018
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| 300 |
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|a 1 - 65
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| 336 |
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|a رسائل جامعية
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| 502 |
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|b رسالة ماجستير
|c جامعة السلطان قابوس
|f كلية العلوم
|g عمان
|o 0603
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| 520 |
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|a X-ray binaries are star systems that emit X-rays. They are among the brightest sources of X-rays in the Galaxy. We have used a simulation software to produce optical and X-ray light curves for different wavelength ranges of light, while adding a sine wave of varying frequency and random noise to the light curves of the binary star system. Variations in these light curves can give important clues on both the geometry of the system as well as the physical processes that produce them. We also produced Fourier Spectra for the Fourier Transforms of these light curves, and finally, we have produced Fourier resolved spectra for the simulated light curves. Our main purpose is to explore the variability structure of the varying wavelengths of light from X-ray binaries. Using the simulated Fourier Resolved Spectra, we investigate the time variability and study the behaviour of the light curves of different energy and frequency bands.
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| 653 |
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|a التحليل الطيفي
|a الأنظمة النجمية
|a الأشعة السينية
|a برامج المحاكاة
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| 700 |
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|9 509614
|a Ioannou, Zacharias
|e Advisor
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| 700 |
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|a Ibrahim, Alaa I.
|e Advisor
|9 520457
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| 856 |
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|u 9809-008-007-0603-T.pdf
|y صفحة العنوان
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| 856 |
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|u 9809-008-007-0603-A.pdf
|y المستخلص
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| 856 |
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|u 9809-008-007-0603-C.pdf
|y قائمة المحتويات
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| 856 |
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|u 9809-008-007-0603-F.pdf
|y 24 صفحة الأولى
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| 856 |
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|u 9809-008-007-0603-1.pdf
|y 1 الفصل
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| 856 |
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|u 9809-008-007-0603-2.pdf
|y 2 الفصل
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| 856 |
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|u 9809-008-007-0603-3.pdf
|y 3 الفصل
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| 856 |
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|u 9809-008-007-0603-4.pdf
|y 4 الفصل
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| 856 |
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|u 9809-008-007-0603-5.pdf
|y 5 الفصل
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| 856 |
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|u 9809-008-007-0603-O.pdf
|y الخاتمة
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| 856 |
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|u 9809-008-007-0603-R.pdf
|y المصادر والمراجع
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| 856 |
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|u 9809-008-007-0603-S.pdf
|y الملاحق
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| 930 |
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|d y
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| 995 |
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|a Dissertations
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| 999 |
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|c 1050703
|d 1050703
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