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Studying the gamma- ray emission from the magnetar SGR 1900+ 14 with NASA swift mission / Mona Molham Mostafa Elhalaby ; Supervised Mohammed Abdelaziz Rassem , Alaa Ibrahim Hussein

By: Contributor(s): Material type: TextTextLanguage: English Publication details: Cairo : Mona Molham Mostafa Elhalaby , 2012Description: 104P. : charts , facsimiles ; 25cmOther title:
  • Swift الرصوده بالبعثه الفضائيه SGR 1900=14 دراسة الأشعاعات ذات الطاقات العلية من الماجنيتار [Added title page title]
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  • Issued also as CD
Dissertation note: Thesis (M.Sc.) - Cairo University - Faculty of Science - Department of Astronomy and Meteorology Summary: Magnetars are newly discovered cosmic sources of high engergy radiations that emit short intense bursts of x - rays and {u03D3}-rays. Studying the spectral and temporal properties of these bursts of SGR 1900+14 allows us to identify the physical mechanism responsible for their emission and to probe the interaction of radiation and matter at extreme conditions of temperature gravity and magnetic field that cannot be reproduced in earth - based laboratories or paticle accelerators
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Item type Current library Home library Call number Copy number Status Barcode
Thesis Thesis قاعة الرسائل الجامعية - الدور الاول المكتبة المركزبة الجديدة - جامعة القاهرة Cai01.12.01.M.Sc.2012.Mo.S (Browse shelf(Opens below)) Not for loan 01010110060081000
CD - Rom CD - Rom مخـــزن الرســائل الجـــامعية - البدروم المكتبة المركزبة الجديدة - جامعة القاهرة Cai01.12.01.M.Sc.2012.Mo.S (Browse shelf(Opens below)) 60081.CD Not for loan 01020110060081000

Thesis (M.Sc.) - Cairo University - Faculty of Science - Department of Astronomy and Meteorology

Magnetars are newly discovered cosmic sources of high engergy radiations that emit short intense bursts of x - rays and {u03D3}-rays. Studying the spectral and temporal properties of these bursts of SGR 1900+14 allows us to identify the physical mechanism responsible for their emission and to probe the interaction of radiation and matter at extreme conditions of temperature gravity and magnetic field that cannot be reproduced in earth - based laboratories or paticle accelerators

Issued also as CD

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