A bright off-nuclear X-ray source: a type IIn supernova, a bright ULX or a recoiling supermassive black hole in CXO J122518.6+144545-Reference-Cited by-同舟云学术

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A bright off-nuclear X-ray source: a type IIn supernova, a bright ULX or a recoiling supermassive black hole in CXO J122518.6+144545

Published:2010-06-22 Issue:1 Volume:407 Page:645-650
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Jonker P. G.,Torres M. A. P.,Fabian A. C.,Heida M.,Miniutti G.,Pooley D.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/407/1/645/3090006/mnras0407-0645.pdf

Reference63 articles.

1. A Large, Uniform Sample of X-Ray-emitting Active Galactic Nuclei from theROSATAll Sky and Sloan Digital Sky Surveys: The Data Release 5 Sample

2. Gravitational-Wave Extraction from an Inspiraling Configuration of Merging Black Holes

3. Optical and Infrared Properties of the 2 Ms Chandra Deep Field North X-Ray Sources

4. Massive black hole binaries in active galactic nuclei

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1. Merger-driven Growth of Intermediate-mass Black Holes: Constraints from Hubble Space Telescope Imaging of Hyper-luminous X-Ray Sources;The Astrophysical Journal;2024-03-29

2. CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at 0.6 < z < 1.3;The Astrophysical Journal;2023-01-01

3. Statistical analysis of kicked black holes from TNG300 simulation;Publications of the Astronomical Society of Australia;2023

4. Electromagnetic counterparts to massive black-hole mergers;Living Reviews in Relativity;2022-06-24

5. The Redshift Evolution of Ultraluminous X-Ray Sources out to z ∼ 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background;The Astrophysical Journal;2022-06-01

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