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Photometric Study of some cD Galaxies / Eman Aly Shaban Abdelmotaleb ; Supervised Magdy Youssef Amin , Gamal Bakr Ali

By: Contributor(s): Material type: TextTextLanguage: English Publication details: Cairo : Eman Aly Shaban Abdelmotaleb , 2014Description: 82 P. : charts , facsimiles ; 25cmOther title:
  • (cD) درا{uئإآ٣}{uئإ٩٤} {uئإؤ٣}{uئإإإ}{uئإ٩٧}{uئإإإ}{uئإإ٣}{uئإ٩٨}{uئإءإ}{uئإئ٣}{uئإ٩٤} {uئإؤئ}{uئإ٩٢}{uئإأأ}{uئإآإ} ا{uئإؤئ}{uئإإ٤}{uئإء٠}{uئإءإ}ات {uئإإ٣}{uئإإ٦} ا{uئإؤئ}{uئإإ٨}{uئإإإ}ع [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: In this MSc study, we aim to determine the shape of the surface brightness profile of the extended envelope of a sample of cD galaxies. Both de Vaucouleurs r1/4 low and Sersic's r1/n model, on their own, provide a poor description of the surface brightness profiles of cD galaxies. We therefore plan to determine the most appropriate analytical model to describe cD galaxy, whether this be an exponential profile, a Sersic model, or some other function. We additionally intend to measure the fraction of light contained within their different components. Among others the following will be determined: Luminosity profiles along the major and minor axes, Structural profiles (Position angle profile, ellipticity profile, etc.), Color distribution
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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.2014.Em.P (Browse shelf(Opens below)) Not for loan 01010110065319000
CD - Rom CD - Rom مخـــزن الرســائل الجـــامعية - البدروم المكتبة المركزبة الجديدة - جامعة القاهرة Cai01.12.01.M.Sc.2014.Em.P (Browse shelf(Opens below)) 65319.CD Not for loan 01020110065319000

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

In this MSc study, we aim to determine the shape of the surface brightness profile of the extended envelope of a sample of cD galaxies. Both de Vaucouleurs r1/4 low and Sersic's r1/n model, on their own, provide a poor description of the surface brightness profiles of cD galaxies. We therefore plan to determine the most appropriate analytical model to describe cD galaxy, whether this be an exponential profile, a Sersic model, or some other function. We additionally intend to measure the fraction of light contained within their different components. Among others the following will be determined: Luminosity profiles along the major and minor axes, Structural profiles (Position angle profile, ellipticity profile, etc.), Color distribution

Issued also as CD

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