The XMM-Newton and BeppoSAX view of the ultraluminous infrared galaxy MKN 231
Feb, 200411 pages
Published in:
- Astron.Astrophys. 420 (2004) 79-88
e-Print:
- astro-ph/0402226 [astro-ph]
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Abstract: (arXiv)
We discuss XMM-Newton and BeppoSAX observations of MKN 231, the lowest-redshift Broad Absorption Line (BAL) QSO known so far and one of the best-studied Ultra Luminous Infrared Galaxies. By combining the XMM-Newton spectral resolution and the high-energy bandpass of BeppoSAX we have been able to study in more detail than previously possible its 0.2--50 keV spectral properties. The BeppoSAX PDS data unveiled, for the first time, a highly absorbed (cm) power-law component. We find that: a) below 10 keV we are seeing only reprocessed radiation through reflection and/or scattering: b) the intrinsic 2-10 keV luminosity of MKN 231 is ergs s, i.e. more than an order of magnitude greater than previous measurements: c) the starburst activity significantly contributes to the soft ( keV) X-ray emission.- X-rays: galaxies
- galaxies: individual: Markarian 231
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