Studying the [O iii]λ5007 Å emission-line width in a sample of ∼ 80 local active galaxies: a surrogate for σ⋆?-Reference-Cited by-同舟云学术

Studying the [O iii]λ5007 Å emission-line width in a sample of ∼ 80 local active galaxies: a surrogate for σ⋆?

Published:2018-08-18 Issue:1 Volume:481 Page:138-152
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Bennert Vardha N¹,Loveland Donald¹,Donohue Edward¹,Cosens Maren¹,Lewis Sean¹,Komossa S²,Treu Tommaso³,Malkan Matthew A³,Milgram Nathan¹,Flatland Kelsi¹,Auger Matthew W⁴,Park Daeseong⁵,Lazarova Mariana S⁶

Affiliation:

1. Physics Department, California Polytechnic State University, San Luis Obispo CA 93407, USA

2. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany

3. Department of Physics, University of California, Los Angeles, CA 90095, USA

4. Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK

5. Korea Astronomy and Space Science Institute, Daejeon 34055, Republic of Korea

6. Department of Physics and Astronomy, University of Nebraska Kearney, Kearney, NE 68849, USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/481/1/138/25681398/sty2236.pdf

Reference52 articles.

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5. THE RELATION BETWEEN BLACK HOLE MASS AND HOST SPHEROID STELLAR MASS OUT TOz∼ 2

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