Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23610
Title: | The structure of the X-ray absorber in Mrk 915 revealed by Swift | Authors: | SEVERGNINI, Paola Ballo, L. BRAITO, Valentina CACCIANIGA, Alessandro CAMPANA, Sergio DELLA CECA, Roberto MORETTI, Alberto Vignali, C. |
Issue Date: | 2015 | Journal: | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | Number: | 453 | Issue: | 4 | First Page: | 3611 | Abstract: | In this paper, we present the results obtained with a monitoring programme (23 days long) performed with Swift-XRT on the local Seyfert galaxy Mrk 915. The light-curve analysis shows a significant count rate variation (about a factor of 2-3) on a time-scale of a few days, while the X-ray colours show a change in the spectral curvature below 2 keV and the presence of two main spectral states. From the spectral analysis we find that the observed variations can be explained by the change of the intrinsic nuclear power (about a factor of 1.5) coupled with a change of the properties of an ionized absorber. The quality of the data prevents us from firmly establishing if the spectral variation is due to a change in the ionization state and/or in the covering factor of the absorbing medium. The latter scenario would imply a clumpy structure of the ionized medium. By combining the information provided by the light curve and the spectral analyses, we can derive some constraints on the location of the absorber under the hypotheses of either homogeneous or clumpy medium. In both cases, we find that the absorber should be located inside the outer edge of an extended torus and, in particular, under the clumpy hypothesis, it should be located near, or just outside, to the broad emission line region. | Acknowledgments: | This work is based on observations obtained with the Swift satellite and it made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. We thank Neil Gehrels, Boris Sbarufatti, Gianpiero Tagliaferri and the Swift Mission Operation Center to make every effort to get our ToO request scheduled. This research has made use both of the Palermo BAT Catalogue and database operated at INAF - IASF Palermo and of the 70 month Swift -BAT Catalogue. We, moreover, thank Miguel Perez-Torres for the analysis of archival VLA data. Part of this work was supported by the European Commission Seventh Framework Programme (FP7/2007-2013) under grant agreement no. 267251 Astronomy Fellowships in Italy (AstroFIt). The authors acknowledge financial support from the Italian Ministry of Education, Universities and Research (PRIN2010-2011, grant no. 2010NHBSBE). Support from the Italian Space Agency is acknowledged (contract ASI INAF I/037/12/0). Finally, we you would like to thank the anonymous referee for the useful and constructive comments which improved the quality of the paper. | URI: | http://hdl.handle.net/20.500.12386/23610 | URL: | https://academic.oup.com/mnras/article/453/4/3611/2593681 | ISSN: | 0035-8711 | DOI: | 10.1093/mnras/stv1851 | Bibcode ADS: | 2015MNRAS.453.3611S | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2015MNRAS_453_3611.pdf | 644.02 kB | Adobe PDF | View/Open |
Page view(s)
73
checked on Sep 12, 2024
Download(s)
28
checked on Sep 12, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.