EDP Sciences
Free Access
Volume 407, Number 2, August IV 2003
Page(s) L21 - L24
Section Letters
DOI https://doi.org/10.1051/0004-6361:20031054

A&A 407, L21-L24 (2003)
DOI: 10.1051/0004-6361:20031054


The origin of the iron lines in NGC 7213

S. Bianchi, G. Matt, I. Balestra and G. C. Perola

Dipartimento di Fisica, Università degli Studi Roma Tre, Italy
(Received 20 June 2003 / Accepted 8 July 2003)

The analysis of a simultaneous XMM-Newton/BeppoSAX plus three previous BeppoSAX observations revealed that NGC 7213 is a rather peculiar Seyfert 1. No significant Compton reflection component was observed, while an iron line complex, best explained in terms of three narrow lines, is clearly apparent in the data. Due to the absence of the reflection component, the neutral iron line is likely not produced in a Compton-thick material, but current data do not allow to choose between a Compton-thin torus and the BLR. The two ionized iron lines from $\ion{Fe}{xxv}$ and $\ion{Fe}{xxvi}$ may be produced in a photoionized gas with a column density of a few 10 23 cm -2, in analogy with the case of NGC 5506.

Key words: galaxies: individual: NGC 7213 -- galaxies: Seyfert -- X-rays: galaxies

Offprint request: S. Bianchi, bianchi@fis.uniroma3.it

SIMBAD Objects

© ESO 2003

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.