翻訳と辞書
Words near each other
・ Twin Peaks books
・ Twin Peaks home video releases
・ Twin Peaks Tunnel
・ Twin Peaks Wilderness
・ Twin Peaks, California
・ Twin Pimples raid
・ Twin Pine Airport
・ Twin Pine Casino
・ Twin Pinnacles
・ Twin Poplars, Virginia
・ Twin Ports
・ Twin Ports League
・ Twin Ports Music and Arts Collective
・ Twin prime
・ Twin Prime Search
Twin Quasar
・ Twin Range
・ Twin Registry
・ Twin registry
・ Twin Research and Human Genetics
・ Twin reversed arterial perfusion
・ Twin Ring Motegi
・ Twin River
・ Twin River Casino
・ Twin River Collegiate Conference
・ Twin River Public Schools
・ Twin Rivers
・ Twin Rivers (film)
・ Twin Rivers Adult School
・ Twin Rivers Corrections Center


Dictionary Lists
翻訳と辞書 辞書検索 [ 開発暫定版 ]
スポンサード リンク

Twin Quasar : ウィキペディア英語版
Twin Quasar

The Twin Quasar (''Twin QSO'' or Double Quasar or ''Old Faithful'', also known as SBS 0957+561, TXS 0957+561, Q0957+561 or QSO 0957+561 A/B), was discovered in 1979 and was the first identified gravitationally lensed object. It is a quasar that appears as two images, a result from gravitational lensing caused by the galaxy YGKOW G1 that is located in the line of sight between Earth and the quasar.
==Quasar==
QSO 0957+561 A (SBS 0957+561 A) and QSO 0957+561 B (SBS 0957+561 B) are the two components of a double-imaged quasar, meaning that an intervening mass concentration between Earth and the quasar bends light so that two images of the quasar appear in the sky. This is known as gravitational lensing, and is a consequence of Einsteinian warped space-time. The quasar lies at redshift ''z'' = 1.41 (8.7 billion ly), while the lensing galaxy lies at redshift ''z'' = 0.355 (3.7 billion ly). The lensing galaxy with apparent dimension of 0.42×0.22 arcminutes lies almost in line with the B image, lying 1 arcsecond off. The quasar lies 10 arcminutes north of NGC 3079, in the constellation Ursa Major. The astronomical data services SIMBAD and NASA/IPAC Extragalactic Database (NED) list several other names for this system.
The Twin Quasar's two images are separated by 6 arcseconds. Both images have an apparent magnitude of 17, with the A component having 16.7 and the B component having 16.5. There is a 417 ± 3 day time lag between the two images.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Twin Quasar」の詳細全文を読む



スポンサード リンク
翻訳と辞書 : 翻訳のためのインターネットリソース

Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.