Ultraviolet Fe ii emission in fainter quasars: luminosity dependences, and the influence of environments-Reference-Cited by-同舟云学术

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Ultraviolet Fe ii emission in fainter quasars: luminosity dependences, and the influence of environments

Published:2016-05-01 Issue:2 Volume:460 Page:1428-1444
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Clowes Roger G.,Haberzettl Lutz,Raghunathan Srinivasan,Williger Gerard M.,Mitchell Sophia M.,Söchting Ilona K.,Graham Matthew J.,Campusano Luis E.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/460/2/1428/8115109/stw1021.pdf

Reference94 articles.

1. Luminosity Indicators in the Spectra of Quasi-Stellar Objects

2. Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines

3. The Origin of FeiiEmission in Active Galactic Nuclei

4. THE LICK AGN MONITORING PROJECT 2011: Fe II REVERBERATION FROM THE OUTER BROAD-LINE REGION

5. Baskin A. ASP Conf. Ser. Vol. 460. AGN Winds in Charleston. Chartas G. Hamann F. Leighly K. M. , editors. Astron. Soc. Pac.; San Francisco; 2012. p. 159.

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1. UV FeII emission model of HE 0413−4031 and its relation to broad-line time delays;Astronomy & Astrophysics;2024-03

2. SPT: Spectral transformer for age and mass estimations of red giant stars;Astronomy & Astrophysics;2024-03

3. Extreme quasars at high redshift;Astronomy & Astrophysics;2018-10

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