Open AccessXMM‐Newton discovery of a sharp spectral feature at ∼ 7 keV in the narrow‐line Seyfert 1 galaxy 1H 0707−495
Author(s) -
Boller TH.,
Fabian A.C.,
Sunyaev R.,
Trümper J.,
Vaughan S.,
Ballantyne D.R.,
Brandt W.N.,
Keil R.,
Iwasawa K.
Publication year - 2002
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2002.05040.x
Subject(s) - physics , astrophysics , galaxy , line (geometry) , ionization , spectral line , flux (metallurgy) , emission spectrum , reflection (computer programming) , photoelectric effect , absorption (acoustics) , feature (linguistics) , astronomy , optics , ion , geometry , quantum mechanics , linguistics , philosophy , mathematics , materials science , computer science , metallurgy , programming language
We report the first detection of a sharp spectral feature in a narrow‐line Seyfert 1 galaxy. Using XMM‐Newton we have observed 1H and find a drop in flux by a factor of more than 2 at a rest‐frame energy of ∼ 7 keV without any detectable narrow Fe K α line emission. The energy of this feature suggests a connection with the neutral iron K photoelectric edge, but the lack of any obvious absorption in the spectrum at lower energies makes the interpretation challenging. We explore two alternative explanations for this unusual spectral feature: (i) partial‐covering absorption by clouds of neutral material; and (ii) ionized disc reflection with lines and edges from different ionization stages of iron blurred together by relativistic effects. We note that both models require an iron overabundance to explain the depth of the feature. The X‐ray light curve shows strong and rapid variability, changing by a factor of 4 during the observation. The source displays modest spectral variability which is uncorrelated with flux.