Repository logo
  • English
  • 中文
Log In
Have you forgotten your password?
  1. Home
  2. College of Science / 理學院
  3. Astrophysics / 天文物理研究所
  4. KK258, a new transition dwarf galaxy neighbouring the local group
 
  • Details

KK258, a new transition dwarf galaxy neighbouring the local group

Journal
Monthly Notices of the Royal Astronomical Society
Journal Volume
443
Journal Issue
2
Pages
1281-1290
Date Issued
2014
Author(s)
Karachentsev I.D
Makarova L.N
Tully R.B
PO-FENG WU  
Kniazev A.Y.
DOI
10.1093/mnras/stu1217
URI
https://www.scopus.com/inward/record.uri?eid=2-s2.0-84905658602&doi=10.1093%2fmnras%2fstu1217&partnerID=40&md5=d49d5b7ec85ca1c270a284fd4f857d8b
https://scholars.lib.ntu.edu.tw/handle/123456789/624943
Abstract
Here, we present observations with the Advanced Camera for Surveys on the Hubble Space Telescope of the nearby, transition-type dwarf galaxy KK258 = ESO468-020. We measure a distance of 2.23 ± 0.05 Mpc using the Tip of Red Giant Branch method. We also detect Ha emission from this gas-poor dwarf transition galaxy at the velocity Vh = 92 ± 5 or VLG = 150 km s-1.With this distance and velocity, KK258 lies near the local Hubble flow locus with a peculiar velocity ∼3 km s-1. We discuss the star formation history of KK258 derived from its colour-magnitude diagram. The specific star formation rate is estimated to be log[sSFR] = -2.64 and -2.84 (Gyr-1) from the FUV-flux and Ha-flux, respectively. KK258 has the absolute magnitude MB = -10.3 mag, the average surface brightness of 26.0 mag arcsec-2 and the hydrogen mass log(MHI) < 5.75M⊙.We compare KK258 with 29 other dTr- galaxies situated within 5 Mpc from us, and conclude that its properties are typical for transition dwarfs. However, KK258 resides 0.8 Mpc away from its significant neighbour, the Sdm galaxy NGC 55, and such a spatial isolation is unusual for the local transition dwarfs. © 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
Subjects
Galaxies: distances and redshifts; Galaxies: dwarf; Galaxies: individual: KK258; Galaxies: stellar content
Other Subjects
Giant stars; Advanced camera for surveys; Dwarf galaxies; Galaxies distances and redshifts; Galaxies: dwarf; Galaxies: individuals; Galaxy: individual: kk258; Galaxy:stellar content; Hubble space telescopes; Local groups; Red giant branches; Galaxies
Type
journal article

臺大位居世界頂尖大學之列,為永久珍藏及向國際展現本校豐碩的研究成果及學術能量,圖書館整合機構典藏(NTUR)與學術庫(AH)不同功能平台,成為臺大學術典藏NTU scholars。期能整合研究能量、促進交流合作、保存學術產出、推廣研究成果。

To permanently archive and promote researcher profiles and scholarly works, Library integrates the services of “NTU Repository” with “Academic Hub” to form NTU Scholars.

總館學科館員 (Main Library)
醫學圖書館學科館員 (Medical Library)
社會科學院辜振甫紀念圖書館學科館員 (Social Sciences Library)

開放取用是從使用者角度提升資訊取用性的社會運動,應用在學術研究上是透過將研究著作公開供使用者自由取閱,以促進學術傳播及因應期刊訂購費用逐年攀升。同時可加速研究發展、提升研究影響力,NTU Scholars即為本校的開放取用典藏(OA Archive)平台。(點選深入了解OA)

  • 請確認所上傳的全文是原創的內容,若該文件包含部分內容的版權非匯入者所有,或由第三方贊助與合作完成,請確認該版權所有者及第三方同意提供此授權。
    Please represent that the submission is your original work, and that you have the right to grant the rights to upload.
  • 若欲上傳已出版的全文電子檔,可使用Open policy finder網站查詢,以確認出版單位之版權政策。
    Please use Open policy finder to find a summary of permissions that are normally given as part of each publisher's copyright transfer agreement.
  • 網站簡介 (Quickstart Guide)
  • 使用手冊 (Instruction Manual)
  • 線上預約服務 (Booking Service)
  • 方案一:臺灣大學計算機中心帳號登入
    (With C&INC Email Account)
  • 方案二:ORCID帳號登入 (With ORCID)
  • 方案一:定期更新ORCID者,以ID匯入 (Search for identifier (ORCID))
  • 方案二:自行建檔 (Default mode Submission)
  • 方案三:學科館員協助匯入 (Email worklist to subject librarians)

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science