A highly polarized radio jet during the 1998 outburst of the black hole transient XTE J1748-288

XTE J1748-288 is a black hole X-ray transient which went into outburst in 1998 June. The X-ray light curves showed canonical morphologies, with minor variations on the `fast rise exponential decay' profile. The radio source, however, reached an unusually high flux density of over 600 mJy. This...

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Main Authors: Brocksopp, C., Miller-Jones, James, Fender, R., Stappers, B.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2007
Subjects:
Online Access:http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2007.11846.x/full
http://hdl.handle.net/20.500.11937/41938
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author Brocksopp, C.
Miller-Jones, James
Fender, R.
Stappers, B.
author_facet Brocksopp, C.
Miller-Jones, James
Fender, R.
Stappers, B.
author_sort Brocksopp, C.
building Curtin Institutional Repository
collection Online Access
description XTE J1748-288 is a black hole X-ray transient which went into outburst in 1998 June. The X-ray light curves showed canonical morphologies, with minor variations on the `fast rise exponential decay' profile. The radio source, however, reached an unusually high flux density of over 600 mJy. This high radio flux was accompanied by an exceptional (>20 per cent) fractional linear polarization, the variability of which was anticorrelated with the flux density. We use this variability to discuss possible depolarization mechanisms and to predict the underlying behaviour of the (unresolved) core/jet components.
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T09:09:43Z
publishDate 2007
publisher Wiley-Blackwell Publishing Ltd.
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spelling curtin-20.500.11937-419382019-02-19T04:27:41Z A highly polarized radio jet during the 1998 outburst of the black hole transient XTE J1748-288 Brocksopp, C. Miller-Jones, James Fender, R. Stappers, B. accretion stars: individual: XTE J1748-288 accretion discs X-rays: binaries ISM: jets and outflows XTE J1748-288 is a black hole X-ray transient which went into outburst in 1998 June. The X-ray light curves showed canonical morphologies, with minor variations on the `fast rise exponential decay' profile. The radio source, however, reached an unusually high flux density of over 600 mJy. This high radio flux was accompanied by an exceptional (>20 per cent) fractional linear polarization, the variability of which was anticorrelated with the flux density. We use this variability to discuss possible depolarization mechanisms and to predict the underlying behaviour of the (unresolved) core/jet components. 2007 Journal Article http://hdl.handle.net/20.500.11937/41938 http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2007.11846.x/full Wiley-Blackwell Publishing Ltd. restricted
spellingShingle accretion
stars: individual: XTE J1748-288
accretion discs
X-rays: binaries
ISM: jets and outflows
Brocksopp, C.
Miller-Jones, James
Fender, R.
Stappers, B.
A highly polarized radio jet during the 1998 outburst of the black hole transient XTE J1748-288
title A highly polarized radio jet during the 1998 outburst of the black hole transient XTE J1748-288
title_full A highly polarized radio jet during the 1998 outburst of the black hole transient XTE J1748-288
title_fullStr A highly polarized radio jet during the 1998 outburst of the black hole transient XTE J1748-288
title_full_unstemmed A highly polarized radio jet during the 1998 outburst of the black hole transient XTE J1748-288
title_short A highly polarized radio jet during the 1998 outburst of the black hole transient XTE J1748-288
title_sort highly polarized radio jet during the 1998 outburst of the black hole transient xte j1748-288
topic accretion
stars: individual: XTE J1748-288
accretion discs
X-rays: binaries
ISM: jets and outflows
url http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2007.11846.x/full
http://hdl.handle.net/20.500.11937/41938