Determination of the size of the dust torus in H0507+164 through optical and infrared monitoring-Reference-Cited by-同舟云学术

Determination of the size of the dust torus in H0507+164 through optical and infrared monitoring

Published:2018-01-29 Issue:4 Volume:475 Page:5330-5337
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Mandal Amit Kumar¹²,Rakshit Suvendu²³,Kurian Kshama S²,Stalin C S²,Mathew Blesson¹,Hoenig Sebastian⁴,Gandhi Poshak⁴^ORCID,Sagar Ram²,Pandge M B⁵^ORCID

Affiliation:

1. Department of Physics, Christ University, Hosur Road, Bangalore 560 029, India

2. Indian Institute of Astrophysics, Block II, Koramangala, Bangalore 560 034, India

3. Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Republic of Korea

4. Department of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK

5. Dayanand Science College, Barshi Road, Latur, Maharashtra 413512, India

Funder

Horizon 2020

STFC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/475/4/5330/24106727/sty200.pdf

Reference48 articles.

1. Unified Models for Active Galactic Nuclei and Quasars

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

3. Hot dust and the near-infrared bump in the continuum spectra of quasars and active galactic nuclei

4. The AGN Black Hole Mass Database

5. A Reverberation‐based Mass for the Central Black Hole in NGC 4151

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