EDP Sciences
Free Access
Volume 388, Number 1, June II 2002
Page(s) L5 - L8
Section Letters
DOI https://doi.org/10.1051/0004-6361:20020534
Published online 28 May 2002

A&A 388, L5-L8 (2002)
DOI: 10.1051/0004-6361:20020534


A rapidly variable narrow X-ray iron line in Mkn 841

P. O. Petrucci1, G. Henri1, L. Maraschi2, P. Ferrando3, G. Matt4, M. Mouchet5, C. Perola4, S. Collin5, A. M. Dumont5, F. Haardt6 and L. Koch-Miramond3

1  Laboratoire d'Astrophysique de Grenoble, BP 43, 38041 Grenoble Cedex 9, France
2  Osservatorio Astronomico di Brera, via Brera 28, 02121 Milano, Italy
3  Service d'Astrophysique, DSM/DAPNIA/SAp, CE Saclay, 91191 Gif-sur-Yvette Cedex, France
4  Dipartimento di Fisica, Università degli Studi "Roma tre", via della Vasca Navale 84, 00046 Roma, Italy
5  LUTH, Observatoire de Paris, Section de Meudon, 92195 Meudon Cedex, France
6  Università dell'Insubria, via Lucini 3, 22100 Como, Italy

(Received 26 February 2002 / Accepted 5 April 2002 )

We report on the detection of a rapidly variable narrow Fe K $\alpha$ line in Mkn 841. The source has been observed two times by XMM-Newton and simultaneously with BeppoSAX. The two observations, of about 10 ks long each, were separated by ~15 hours. The line flux reaches a maximum during the first observation and is significantly reduced in the second one. The continuum shape and flux, instead, keep roughly constant between the two pointings. Such rapid variability of a narrow (unresolved by the XMM-pn instrument) line has never been reported in the past. These results are not easily explained in the standard cold reflection model where the narrow line component is supposed to be produced far from the primary X-ray source (e.g. from the torus) and is thus not expected to vary rapidly. Different interpretations are discussed.

Key words: galaxies: individual: Mkn 841 -- galaxies: Seyfert -- X-rays: galaxies

Offprint request: P. O. Petrucci, petrucci@obs.ujf-grenoble.fr

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© ESO 2002

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