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New candidate member and kinematic study of young open clusters IC 348 and NGC 3680 / Mostafa Mahmoud Elnazer ; Supervised Magdy Yousef Amin , Adel Shehata Soliman , Mohamed Nader Ismail

By: Contributor(s): Material type: TextTextLanguage: English Publication details: Cairo : Mostafa Mahmoud Elnazer , 2012Description: 123 P. : charts , facsimiles ; 25cmOther title:
  • IC 348, NGC 3680 عضو مرشح جديد ودراسة لدناميكا المجرت المفتوحة حديثة التكوين [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: Relative cluster membership probabilities have been determined for 2711 stars in a region containing the open cluster NGC 3680 and 1431 stars in the region containing the open cluster IC 348. A Pruning procedure has been carried out to identify the cluster members and the field members, three filtration steps have been processed to determine the member stars and eliminate the field stars, and revealed that 585 stars around the center (11h 25m 34s.67 - 43{u00B0} 13' 37".56) and 464 stars around the center (3h 44m 22s.92 - 32{u00B0} 21' 54".35) are cluster members in NGC 3680 and IC 348 respectively
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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.N (Browse shelf(Opens below)) Not for loan 01010110063457000
CD - Rom CD - Rom مخـــزن الرســائل الجـــامعية - البدروم المكتبة المركزبة الجديدة - جامعة القاهرة Cai01.12.01.M.Sc.2012.Mo.N (Browse shelf(Opens below)) 63457.CD Not for loan 01020110063457000

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

Relative cluster membership probabilities have been determined for 2711 stars in a region containing the open cluster NGC 3680 and 1431 stars in the region containing the open cluster IC 348. A Pruning procedure has been carried out to identify the cluster members and the field members, three filtration steps have been processed to determine the member stars and eliminate the field stars, and revealed that 585 stars around the center (11h 25m 34s.67 - 43{u00B0} 13' 37".56) and 464 stars around the center (3h 44m 22s.92 - 32{u00B0} 21' 54".35) are cluster members in NGC 3680 and IC 348 respectively

Issued also as CD

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