Is there a UV/X-ray connection in IRAS 13224−3809?-Reference-Cited by-同舟云学术

Is there a UV/X-ray connection in IRAS 13224−3809?

Published:2018-01-05 Issue:2 Volume:475 Page:2306-2313
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Buisson D J K,Lohfink A M,Alston W N,Cackett E M,Chiang C-Y^ORCID,Dauser T^ORCID,De Marco B,Fabian A C,Gallo L C,García J A,Jiang J^ORCID,Kara E,Middleton M J,Miniutti G,Parker M L^ORCID,Pinto C^ORCID,Uttley P,Walton D J,Wilkins D R^ORCID

Funder

ERC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/475/2/2306/23730087/sty008.pdf

Reference76 articles.

1. Ultraviolet and X-ray variability of NGC 4051 over 45 days with XMM-Newton and Swift

2. Investigating a fluctuating-accretion model for the spectral-timing properties of accreting black hole systems

3. X-ray to UV variability correlation in MCG–6-30-15

4. ROSAT monitoring of persistent giant and rapid variability in the narrow-line Seyfert 1 galaxy IRAS 13224-3809

5. Ultraviolet and X-ray variability of active galactic nuclei withSwift

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