Volume 397, Number 3, January III 2003
|Page(s)||883 - 890|
|Published online||21 January 2003|
observations of the Seyfert 1 galaxy NGC 3227
Research and Scientific Support Department, European Space Agency – Postbus 299, 2200 AG Noordwijk, The Netherlands
Corresponding author: P. Gondoin, firstname.lastname@example.org
Accepted: 30 October 2002
We report on an XMM–Newton observation of the Seyfert 1 galaxy NGC 3227 performed in November 2000. The observed X-ray spectrum above 4 keV is well fitted by a hard power law continuum () and an absorption edge at 7.6 keV. An Fe K emission line with an equivalent width of 213 eV is detected at 6.4 keV. The line is narrow suggesting contribution from material in low ionization states (<Fe XVII) relatively far from a central black hole. The continuum is strongly absorbed at soft energies by a column of neutral gas ( cm-2) larger than previously measured and covering a significant fraction (≈90%) of the central source. The soft X-ray continuum is also attenuated due to the presence of ionized material ( erg s-1 cm) suggesting the presence of a substantial amount of gas ( cm-2) in the vicinity (<0.4 pc) of the nucleus. We find that NGC 3227 exhibits significant spectral variability above 2 keV on time scales of a few ksec during the XMM–Newton observations. This short term variability is likely related to variation in the continuum emission. Comparisons with previous observations indicate that variability on timescale of a month also involves a change in the column densities of neutral absorbing material along the line of sight to the nucleus.
Key words: galaxies: individual: NGC 3227 / galaxies: nuclei / galaxies: Seyfert
© ESO, 2003
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