UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

Multiwavelength campaign on Mrk 509: testing realistic comptonization models

Branduardi Raymont, G; Petrucci, PO; Paltani, S; Malzac, J; Kaastra, J; Cappi, M; Ponti, G; ... Lubinski, P; + view all (2012) Multiwavelength campaign on Mrk 509: testing realistic comptonization models. In: Proceedings of 'An INTEGRAL view of the high-energy sky (the first 10 years)' - 9th INTEGRAL Workshop and celebration of the 10th anniversary of the launch (INTEGRAL 2012). (pp. -). Green open access

[thumbnail of INTEGRAL 2012_063.pdf]
Preview
PDF
INTEGRAL 2012_063.pdf
Available under License : See the attached licence file.

Download (1MB)

Abstract

Mrk 509 was observed by XMM-Newton and INTEGRAL in October/November 2009, with one observation every four days for a total of ten observations. Each observation has been fitted with a realistic thermal Comptonization model for the continuum emission. Prompted by the correlation between the UV and soft X-ray flux, we used a thermal Comptonization component for the soft X-ray excess. The UV to X-ray/gamma-ray emission of Mrk 509 can be well fitted by these components, pointing to the existence of a hot (kT ∼ 100 keV), optically-thin (τ ∼ 0.5) corona producing the primary continuum. In contrast, the soft X-ray component requires a warm (kT ∼ 1 keV), optically-thick (τ ∼ 10-20) plasma. Estimates of the amplification ratio for this warm plasma support a configuration relatively close to the “theoretical” configuration of a slab corona above a passive disk. This plasma could be the warm upper layer of the accretion disk. In contrast, the hot corona has a more photon-starved geometry. The high temperature (∼ 100 eV) of the soft-photon field entering and cooling it favors a localization of the hot corona in the inner flow. This soft-photon field could be part of the comptonized emission produced by the warm plasma.

Type: Proceedings paper
Title: Multiwavelength campaign on Mrk 509: testing realistic comptonization models
Event: Integral 2012: An INTEGRAL view of the high-energy sky (the first 10 years) - 9th INTEGRAL Workshop and celebration of the 10th anniversary of the launch
Location: Paris, France
Dates: 2012-10-15 - 2012-10-19
Open access status: An open access version is available from UCL Discovery
Publisher version: http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid...
Language: English
Additional information: © 2012 The Authors. Publication available under a Creative Commons Attribution-Noncommercial-Share Alike 3.0 licence (CC BY-NC-SA) described at http://creativecommons.org/licenses/by-nc-sa/3.0/.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/1420273
Downloads since deposit
99Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item