ログイン
言語:

WEKO3

  • トップ
  • ランキング
To
lat lon distance
To

Field does not validate



インデックスリンク

インデックスツリー

メールアドレスを入力してください。

WEKO

One fine body…

WEKO

One fine body…

アイテム

  1. 学術雑誌論文等

First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole

https://hiroshima.repo.nii.ac.jp/records/2008902
https://hiroshima.repo.nii.ac.jp/records/2008902
544b9fd2-9b6f-4a50-abe7-bdae1dd404fb
名前 / ファイル ライセンス アクション
ApJL_875_L1.pdf ApJL_875_L1.pdf (2.5 MB)
Item type デフォルトアイテムタイプ_(フル)(1)
公開日 2023-03-18
タイトル
タイトル First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
言語 en
作成者 The Event Horizon Telescope Collaboration

× The Event Horizon Telescope Collaboration

en The Event Horizon Telescope Collaboration

Search repository
Sasada, Mahito

× Sasada, Mahito

en Sasada, Mahito

Search repository
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
権利情報
権利情報 © 2019. The American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
主題
主題Scheme Other
主題 accretion
主題
主題Scheme Other
主題 accretion disks
主題
主題Scheme Other
主題 black hole physics
主題
主題Scheme Other
主題 galaxies: active
主題
主題Scheme Other
主題 galaxies: individual (M87)
主題
主題Scheme Other
主題 galaxies: jets
主題
主題Scheme Other
主題 gravitation
内容記述
内容記述 When surrounded by a transparent emission region, black holes are expected to reveal a dark shadow caused by gravitational light bending and photon capture at the event horizon. To image and study this phenomenon, we have assembled the Event Horizon Telescope, a global very long baseline interferometry array observing at a wavelength of 1.3 mm. This allows us to reconstruct event-horizon-scale images of the supermassive black hole candidate in the center of the giant elliptical galaxy M87. We have resolved the central compact radio source as an asymmetric bright emission ring with a diameter of 42±3μas, which is circular and encompasses a central depression in brightness with a flux ratio ≳10:1. The emission ring is recovered using different calibration and imaging schemes, with its diameter and width remaining stable over four different observations carried out in different days. Overall, the observed image is consistent with expectations for the shadow of a Kerr black hole as predicted by general relativity. The asymmetry in brightness in the ring can be explained in terms of relativistic beaming of the emission from a plasma rotating close to the speed of light around a black hole. We compare our images to an extensive library of ray-traced general-relativistic magnetohydrodynamic simulations of black holes and derive a central mass of M=(6.5±0.7)×10⁹M_⊙. Our radio-wave observations thus provide powerful evidence for the presence of supermassive black holes in centers of galaxies and as the central engines of active galactic nuclei. They also present a new tool to explore gravity in its most extreme limit and on a mass scale that was so far not accessible.
言語 en
出版者
出版者 The American Astronomical Society
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_6501
資源タイプ journal article
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
関連情報
識別子タイプ DOI
関連識別子 10.3847/2041-8213/ab0ec7
関連情報
識別子タイプ DOI
関連識別子 https://doi.org/10.3847/2041-8213/ab0ec7
収録物識別子
収録物識別子タイプ ISSN
収録物識別子 2041-8205
収録物識別子
収録物識別子タイプ ISSN
収録物識別子 2041-8213
開始ページ
開始ページ L1
書誌情報 The Astrophysical Journal Letters
The Astrophysical Journal Letters

巻 875, 号 1, p. L1, 発行日 2019-04-10
旧ID 48224
戻る
0
views
See details
Views

Versions

Ver.1 2025-02-21 04:38:32.616445
Show All versions

Share

Mendeley Twitter Facebook Print Addthis

Cite as

エクスポート

OAI-PMH
  • OAI-PMH JPCOAR 2.0
  • OAI-PMH JPCOAR 1.0
  • OAI-PMH DublinCore
  • OAI-PMH DDI
Other Formats
  • JSON
  • BIBTEX

Confirm


Powered by WEKO3


Powered by WEKO3