博碩士論文 109222040 完整後設資料紀錄

DC 欄位 語言
DC.contributor物理學系zh_TW
DC.creator譚學深zh_TW
DC.creatorHok-Sum Tamen_US
dc.date.accessioned2024-7-25T07:39:07Z
dc.date.available2024-7-25T07:39:07Z
dc.date.issued2024
dc.identifier.urihttp://ir.lib.ncu.edu.tw:444/thesis/view_etd.asp?URN=109222040
dc.contributor.department物理學系zh_TW
DC.description國立中央大學zh_TW
DC.descriptionNational Central Universityen_US
dc.description.abstract我對悉尼澳大利亞天文台(SAMI)星系巡天中的空間分辨運動學剖面進行了調查,涵蓋了 SAMI 第三輪釋出的數據中八個星系團的多目標積分視場光譜儀測量數據。我的分析集中在成員橢圓星系的一維運動學分佈,透過 IFS 檢查其內在的星系屬性。在我的初步研究中,我辨識了八個星系團中的 12 個最亮星系團星系,並將 127 個橢圓星系的速度彌散分佈分類為四個不同的組別:平坦型、下降型、上升型和不規則型。結合總恆星質量,透過 Jeans 方程式和 Hernquist 模型估算每個星系的視線速度彌散分佈。一個顯著的觀察是,許多最亮星系團星系(BCGs)主要表現出平坦的速度彌散分佈。此外,許多橢圓星系則具有下降的分佈vizh_TW
dc.description.abstractI conducted an investigation of spatially resolved kinematic profiles within the Sydney-Australian-Astronomical-Observatory (SAMI) galaxy survey, encompassing Multi-object Integral-Field Spectrograph measurements across eight galaxy clusters in the SAMI Date Released 3. My analysis focused on the one-dimensional kinematic profiles of member elliptical galaxies, examining their intrinsic galactic properties through IFS. In my preliminary study, I identified the 12 biggest cluster galaxies within eight clusters and categorized the velocity dispersion profiles of 127 elliptical galaxies into four distinct groups: flat, declining, ascending, and irregular (or unclassified). With the total stellar mass, the line-of-sight velocity dispersion profile of each galaxy is estimated by the Jean equation with Hernquist model. A notable observation was that many brightest cluster galaxies predominantly exhibited flat velocity dispersion profiles. Also, many elliptical galaxies have declining profiles.en_US
DC.subject星系團zh_TW
DC.subject橢圓星系zh_TW
DC.subject最亮星系團星系zh_TW
DC.subject速度彌散度zh_TW
DC.subjectClusteren_US
DC.subjectElliptical galaxiesen_US
DC.subjectBiggest cluster galaxiesen_US
DC.subjectVelocity dispersionen_US
DC.title探索星系團中成員星系的空間分辨運動學zh_TW
dc.language.isozh-TWzh-TW
DC.titleExploring Spatially Resolved Kinematics of Member Galaxies in Galaxy Clustersen_US
DC.type博碩士論文zh_TW
DC.typethesisen_US
DC.publisherNational Central Universityen_US

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