X‐Ray Cluster Associated with thez= 1.063 CSS Quasar 3C 186: The Jet is Not Frustrated-Reference-Cited by-同舟云学术

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X‐Ray Cluster Associated with thez= 1.063 CSS Quasar 3C 186: The Jet is Not Frustrated

Published:2005-10-10 Issue:1 Volume:632 Page:110-121
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Siemiginowska Aneta,Cheung C. C.,LaMassa Stephanie,Burke D. J.,Aldcroft Thomas L.,Bechtold Jill,Elvis Martin,Worrall D. M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference90 articles.

1. Evolutionary models for radio sources from compact sources to classical doubles

2. Abundances of the elements: Meteoritic and solar

3. The cluster environments of radio-loud quasars at 0.6 < z < 1.1

4. X-ray spectral evolution of high redshift quasars

5. An XMM-Newton study of the sub-structure in M 87's halo

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1. The Host Galaxy of the Recoiling Black Hole Candidate in 3C 186: An Old Major Merger Remnant at the Center of a z = 1 Cluster;The Astrophysical Journal;2022-06-01

2. The eROSITA Final Equatorial-Depth Survey (eFEDS);Astronomy & Astrophysics;2022-05

3. NOEMA observations support a recoiling black hole in 3C 186;Astronomy & Astrophysics;2022-05

4. 1321+045: A compact steep‐spectrum radio source in a cool‐core galaxy cluster;Astronomische Nachrichten;2021-10-20

5. The Unusual Weak-line Quasar PG1407+265 and Its Foreground z ∼ 0.7 X-Ray Cluster;The Astrophysical Journal;2021-09-01

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