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A High Signal-To-Noise Ultraviolet Spectrum of NGC 7469: New Support for Reprocessing of Continuum RadiationFrom 1996 June 10 to 1996 July 29, the International AGN Watch monitored the Seyfert 1 galaxy NGC 7469 using the International Ultraviolet Explorer, the Rossi X-Ray Timing Explorer, and a network of ground-based observatories. On 1996 June 18, in the midst of this intensive monitoring period, we obtained a high signal-to-noise snapshot of the UV spectrum from 1150 to 3300 A, using the Faint Object Spectrograph (FOS) on the Hubble Space Telescope. This spectrum allows us to disentangle the UV continuum more accurately from the broad wings of the emission lines, to identify clean continuum windows free of contaminating emission and absorption, and to deblend line complexes such as Ly(alpha) + N V, C IV + He II + O III], Si III] + C III], and Mg II + Fe II. Using the FOS spectrum as a template, we have fitted and extracted line and continuum fluxes from the IUE monitoring data. The cleaner continuum extractions c o n h the discovery of time delays between the different UV continuum bands by Wanders et al. Our new measurements show delays increasing with wavelength for continuum bands centered at 1485, 1740, and 1825 A, relative to 1315 A with delays of 0.09, 0.28, and 0.36 days, respectively. Like many other Seyfert I galaxies, the UV spectrum of NGC 7469 shows intrinsic, blue-shifted absorption in Ly(alpha), N V, and C IV. Soft X-ray absorption is also visible in archival ASCA X-ray spectra. The strength of the UV absorption, however, is not compatible with a single-zone model in which the same material absorbs both the UV and X-ray light. Similar to other Seyfert galaxies, such as NGC 3516, the UV-absorbing gas in NGC 7469 has a lower ionization parameter and column density than the X-ray-absorbing material. While the UV and X-ray absorption does not arise in the same material, the frequent occurrence of both associated UV absorption and X-ray warm absorbers in the same galaxies suggests that the gas supply for each has a common origin.
Document ID
20040052875
Acquisition Source
Headquarters
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kriss, Gerard A.
(Space Telescope Science Inst. Baltimore, MD, United States)
Peterson, Bradley M.
(Ohio State Univ. Columbus, OH, United States)
Crenshaw, D. Michael
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Zheng, Wei
(Johns Hopkins Univ. Baltimore, MD, United States)
Date Acquired
August 21, 2013
Publication Date
May 20, 2000
Publication Information
Publication: The Astrophysical Journal
Publisher: American Astronomical Society
Volume: 535
Subject Category
Astrophysics
Funding Number(s)
CONTRACT_GRANT: NAGW-4443
CONTRACT_GRANT: NAG5-8397
CONTRACT_GRANT: NAS5-26555
CONTRACT_GRANT: GO-06747.01-95A
Distribution Limits
Public
Copyright
Other

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