Modelling accretion disc emission with generalized temperature profile and its effect on AGN spectral energy distribution-Reference-Cited by-同舟云学术

Modelling accretion disc emission with generalized temperature profile and its effect on AGN spectral energy distribution

Published:2019-06-04 Issue:3 Volume:487 Page:3884-3903
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Cheng Huaqing¹²^ORCID,Yuan Weimin¹²,Liu He-Yang¹²,Breeveld Alice A³,Jin Chichuan¹,Liu Bifang¹²

Affiliation:

1. Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100101, P. R. China

2. School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, 19A Yuquan Road, Beijing 100049, P. R. China

3. Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK

Funder

National Natural Science Foundation of China

Chinese Academy of Sciences

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1532/28766308/stz1532.pdf

Reference123 articles.

1. Slim accretion disks

2. X-RAY PROPERTIES OF NARROW-LINE SEYFERT 1 GALAXIES WITH VERY SMALL BROADLINE WIDTHS

3. Unified Models for Active Galactic Nuclei and Quasars

4. EVIDENCE THAT MOST TYPE-1 AGNs ARE REDDENED BY DUST IN THE HOST ISM

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