Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Limits on pair production and multizone Comptonization : the broad-band X/γ-ray spectrum of XTE J1550–564 revisited.

Hjalmarsdotter, L. and Axelsson, M. and Done, C. (2016) 'Limits on pair production and multizone Comptonization : the broad-band X/γ-ray spectrum of XTE J1550–564 revisited.', Monthly notices of the Royal Astronomical Society., 456 (4). pp. 4354-4363.

Abstract

At high luminosities black hole binaries show spectra with a strong disc component accompanied by an equally strong tail where at least some of the electrons are non-thermal. We reanalyse the simultaneous ASCA–RXTE–OSSE data from the 1998 outburst of XTE J1550–564, which span 0.7–1000 keV and remain the best data available of a black hole binary in this state. We reassess the importance of electron–positron pair production using a realistically high value of the source compactness for the first time. The lack of an observable annihilation line together with the observed γ-ray flux beyond 511 keV constrains the maximum electron Lorentz factor to be ≤10, and the slope of the injected electrons to ≤2.5. We also use the fast (10–50 Hz) variability spectrum to constrain the spatial dependence of the electron heating and acceleration. We find that the spectrum of the fast variability is consistent with being fully thermal, so that the observed non-thermal emission is produced from further out in the flow.

Item Type:Article
Full text:(VoR) Version of Record
Download PDF
(547Kb)
Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1093/mnras/stv2909
Publisher statement:This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Date accepted:08 December 2015
Date deposited:17 March 2016
Date of first online publication:15 January 2016
Date first made open access:17 March 2016

Save or Share this output

Export:
Export
Look up in GoogleScholar