Soft versus hard X-ray emission in active galactic nuclei: partialcovering and warm-plus-cold absorber models-Reference-Cited by-同舟云学术

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Soft versus hard X-ray emission in active galactic nuclei: partialcovering and warm-plus-cold absorber models

Published:1996-09-11 Issue:2 Volume:282 Page:493-500
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Ceballos M. T.,Barcons X.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/282/2/493/3511147/282-2-493.pdf

Cited by 21 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Redshift evolution of X-ray spectral index of quasars observed by XMM-NEWTON/SDSS;Journal of High Energy Astrophysics;2021-08

2. The interplay between active galactic nuclei and star formation activities of type 1 active galactic nuclei probed by polycyclic aromatic hydrocarbon 3.3 μm emission feature with AKARI;Publications of the Astronomical Society of Japan;2019-02-01

3. A CONNECTION BETWEEN OBSCURATION AND STAR FORMATION IN LUMINOUS QUASARS;The Astrophysical Journal;2015-03-20

4. X-ray absorption and reflection in active galactic nuclei;The Astronomy and Astrophysics Review;2009-03

5. Piecing together the X-ray background: bolometric corrections for active galactic nuclei;Monthly Notices of the Royal Astronomical Society;2007-10-10

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