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Studing the dynamical properties of some galaxy clusters / Mohamed Hamdy Abdullah ; Supervised Mohamed A. Rassem , Gamal B. Ali

By: Contributor(s): Material type: TextTextLanguage: eng Publication details: Cairo : Mohamed Hamdy Abdullah , 2009Description: 110Leaves : charts , facsimiles ; 30cmOther title:
  • دراسة الخصائص الديناميكية لبعض حشود المجرات [Added title page title]
Subject(s): Online resources: Available additional physical forms:
  • Issued also as CD
Dissertation note: Thesis (M.Sc.) - Cairo University - Faculty of Science - Department of Astronomy and Meteorology Summary: Using the DR{u06F7} of SDSS we construct a sample of ٤٢٣٨٢ galaxies with redshifts in the region of 20 galaxy clusters reaching up to {︣u301C} ٥{u٠٠آء} . Using two successive iterative methods the adaptive kernel method and the spherical infall model we obtained {u06F3}{u06F2}٥٦ members belonging to the studied sample . We present the two - dimensional optical map for each cluster using the adaptive kernel method to determine their centers
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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.2009.Mo.S (Browse shelf(Opens below)) Not for loan 01010110052738000
CD - Rom CD - Rom مخـــزن الرســائل الجـــامعية - البدروم المكتبة المركزبة الجديدة - جامعة القاهرة Cai01.12.01.M.Sc.2009.Mo.S (Browse shelf(Opens below)) 52738.CD Not for loan 01020110052738000

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

Using the DR{u06F7} of SDSS we construct a sample of ٤٢٣٨٢ galaxies with redshifts in the region of 20 galaxy clusters reaching up to {︣u301C} ٥{u٠٠آء} . Using two successive iterative methods the adaptive kernel method and the spherical infall model we obtained {u06F3}{u06F2}٥٦ members belonging to the studied sample . We present the two - dimensional optical map for each cluster using the adaptive kernel method to determine their centers

Issued also as CD

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