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Andrew S. Wilson
Researcher at University of Maryland, College Park
Publications - 271
Citations - 15195
Andrew S. Wilson is an academic researcher from University of Maryland, College Park. The author has contributed to research in topics: Galaxy & Radio galaxy. The author has an hindex of 70, co-authored 269 publications receiving 14642 citations. Previous affiliations of Andrew S. Wilson include Liverpool John Moores University & National Council for Scientific and Technological Development.
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Chandra Snapshot Observations of Low-Luminosity Active Galactic Nuclei with a Compact Radio Source
TL;DR: The results of Chandra snapshot observations of 11 low-ionization nuclear emission-line regions (LINERs), three low-luminosity Seyfert galaxies, and one H II-LINER transition object are presented in this article.
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The Difference between Radio-loud and Radio-quiet Active Galaxies
Andrew S. Wilson,Edward Colbert +1 more
TL;DR: In this article, it was shown that the mass and mass accretion rates of radio-loud and radio-quiet active galactic nuclei are not greatly different, and that the difference between the two classes is associated with the spin of the black hole.
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Chandra Snapshot Observations of Low-Luminosity AGNs with a Compact Radio Source
TL;DR: The results of Chandra snapshot observations of 11 LINERs (Low-Ionization Nuclear Emission-line Regions), three low-luminosity Seyfert galaxies, and one HII-LINER transition object are presented in this paper.
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Accretion onto the supermassive black hole in m87
Tiziana Di Matteo,Tiziana Di Matteo,Tiziana Di Matteo,Steven W. Allen,Andrew C. Fabian,Andrew S. Wilson,Andrew J. Young +6 more
TL;DR: In this paper, Chandra X-ray observations of the giant elliptical galaxy M87 resolve the thermal state of the hot interstellar medium into the accretion (Bondi) radius of its central 3 × 109 M☉ black hole.
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Radio sources in low-luminosity active galactic nuclei IV. Radio luminosity function, importance of jet power, and radio properties of the complete Palomar sample
TL;DR: In this paper, a high-resolution radio imaging survey of all low-luminosity active galactic nuclei (LLAGNs) and AGNs in the Palomar Spectroscopic Sample of all (∼488) bright northern galaxies is presented.