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  1. 理工学研究科
  2. 理工学研究科・博士論文

Exploring high precision VLBI astrometry of hydroxyl and water masers to study late stellar evolution

http://hdl.handle.net/10232/00029521
http://hdl.handle.net/10232/00029521
52d16ef4-5095-4447-96e8-60f54106c7e5
名前 / ファイル ライセンス アクション
Diss_Gabor_Orosz_RKK446_2016.pdf Diss_Gabor_Orosz_RKK446_2016 (18.9 MB)
Abstract_Gabor_Orosz_2714530057_2016.pdf Abstract_Gabor_Orosz_2714530057_2016 (129.8 kB)
Result_Gabor_Orosz_rkk446_2016.pdf Result_Gabor_Orosz_rkk446_2016 (79.3 kB)
Comments_Gabor_Orosz_rkk446_2016.pdf Comments_Gabor_Orosz_rkk446_2016 (73.4 kB)
Item type 学位論文 / Thesis or Dissertation(1)
公開日 2017-04-11
タイトル
タイトル Exploring high precision VLBI astrometry of hydroxyl and water masers to study late stellar evolution
別言語のタイトル
その他のタイトル 末期恒星進化研究のための水酸基及び水メーザー源に対する超長基線電波干渉法による高精度天体位置計測
著者 OROSZ, Gabor

× OROSZ, Gabor

WEKO 123987

OROSZ, Gabor

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言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_db06
資源タイプ doctoral thesis
アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
要約(Abstract)
内容記述タイプ Other
内容記述 This PhD thesis has two main topics: technical studies of VLBI astrometry at L-band and astrometric measurements of OH and H2O masers to study late stellar evolution. The technical studies focus on mitigating spatial systematic errors caused by the ionosphere, the bane of VLBI measurements at low-frequencies, which hinder the astrometric applicability of one of the best stellar tracers, 1.6 GHzOH masers. We need to figure out how to do precise astrometry of OH masers; doing this would make it possible to measure accurate distances to evolved stars with heavy dust shells and high mass loss rates, the lack of which impeded on the better understanding of stellar evolution for far too long. This work provides an overview of relative VLBI astrometry from the point of view of error analysis, then goes on to demonstrate new calibration and analysis methods to achieve high precision astrometry at L-band. Some OH maser parallaxes are also measured in the process, but their application to study stellar evolution is ongoing. Additionally, the first results related to H2O masers in the fast outflows of water fountain stars are also presented, with a focus on better understanding the evolutionary process between evolved stars and planetary nebulae.
作成日
日付 2017-03-31
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
NDC
主題Scheme NDC
主題 441.4
ファイル(説明)
内容記述タイプ Other
内容記述 博士論文全文
ファイル(説明)
内容記述タイプ Other
内容記述 博士論文要旨
ファイル(説明)
内容記述タイプ Other
内容記述 最終試験結果の要旨
ファイル(説明)
内容記述タイプ Other
内容記述 論文審査の要旨
公開者・出版者
出版者 鹿児島大学
公開者よみ
公開者よみ カゴシマ ダイガク
公開者別名
公開者別名 Kagoshima University
備考
備考 【指導教員: 今井裕】
学位名
学位名 博士(理学)Doctor of Philosophy in Science
学位授与機関
学位授与機関識別子Scheme kakenhi
学位授与機関識別子 17701
学位授与機関名 鹿児島大学
学位授与年月日
学位授与年月日 2017-03-24
学位授与番号
学位授与番号 甲理工研第446号
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