Swift Monitoring of NGC 4151: Evidence for a Second X-Ray/UV Reprocessing
Swift monitoring of NGC 4151 with an similar to 6 hr sampling over a total of 69 days in early 2016 is used to construct light curves covering five bands in the X-rays (0.3-50 keV) and six in the ultraviolet (UV)/optical (1900-5500 angstrom). The three hardest X-ray bands (> 2.5 keV) are all stro...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Language: | en |
Published: |
IOP PUBLISHING LTD
2017
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Subjects: | |
Online Access: | http://hdl.handle.net/10150/624341 http://arizona.openrepository.com/arizona/handle/10150/624341 |