Isolating the jet in broadband spectra of XBs

Fraser Lewis; David M. Russell; Dipankar Maitra; Robert J.H. Dunn; Sera Markoff; Peter G. Jonker; Manuel Linares; Valeriu Tudose

doi:10.1017/S1743921310016285

Isolating the jet in broadband spectra of XBs

Fraser Lewis, David M. Russell, Dipankar Maitra, Robert J.H. Dunn, Sera Markoff, Peter G. Jonker, Manuel Linares, Valeriu Tudose

Faculty of Life Sciences and Education

Research output: Contribution to journal › Article › peer-review

Abstract

Most accretion-powered relativistic jet sources in our Galaxy are transient X-ray binaries (XBs). Efforts to coordinate multiwavelength observations of these objects have improved dramatically over the last decade. Now the challenge is to interpret broadband spectral energy distributions (SEDs) of XBs that are well sampled in both wavelength and time. Here we focus on the evolution of the jet in their broadband spectra. Some of the most densely sampled broadband SEDs of a neutron star transient (IGR J00291+5934) are used to constrain the optically thick-thin break in the jet spectrum. For the black hole transient XTE J1550-564, infrared - X-ray correlations, evolution of broadband spectraand timing signatures indicate that synchrotron emission from the jet likely dominates the X-ray power law at low luminosities during the hard state outburst decline.

Original language	English
Pages (from-to)	317 - 318
Number of pages	1
Journal	Proceedings of the International Astronomical Union
Volume	6
DOIs	https://doi.org/10.1017/S1743921310016285
Publication status	E-pub ahead of print - 24 Feb 2011

Keywords

accretion
accretion discs
x-rays
binaries
ism
jets and outflows

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10.1017/S1743921310016285

Cite this

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title = "Isolating the jet in broadband spectra of XBs",

abstract = "Most accretion-powered relativistic jet sources in our Galaxy are transient X-ray binaries (XBs). Efforts to coordinate multiwavelength observations of these objects have improved dramatically over the last decade. Now the challenge is to interpret broadband spectral energy distributions (SEDs) of XBs that are well sampled in both wavelength and time. Here we focus on the evolution of the jet in their broadband spectra. Some of the most densely sampled broadband SEDs of a neutron star transient (IGR J00291+5934) are used to constrain the optically thick-thin break in the jet spectrum. For the black hole transient XTE J1550-564, infrared - X-ray correlations, evolution of broadband spectraand timing signatures indicate that synchrotron emission from the jet likely dominates the X-ray power law at low luminosities during the hard state outburst decline.",

keywords = "accretion, accretion discs, x-rays, binaries, ism, jets and outflows",

author = "Fraser Lewis and Russell, {David M.} and Dipankar Maitra and Dunn, {Robert J.H.} and Sera Markoff and Jonker, {Peter G.} and Manuel Linares and Valeriu Tudose",

year = "2011",

month = feb,

day = "24",

doi = "10.1017/S1743921310016285",

language = "English",

volume = "6",

pages = "317 -- 318",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

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TY - JOUR

T1 - Isolating the jet in broadband spectra of XBs

AU - Lewis, Fraser

AU - Russell, David M.

AU - Maitra, Dipankar

AU - Dunn, Robert J.H.

AU - Markoff, Sera

AU - Jonker, Peter G.

AU - Linares, Manuel

AU - Tudose, Valeriu

PY - 2011/2/24

Y1 - 2011/2/24

N2 - Most accretion-powered relativistic jet sources in our Galaxy are transient X-ray binaries (XBs). Efforts to coordinate multiwavelength observations of these objects have improved dramatically over the last decade. Now the challenge is to interpret broadband spectral energy distributions (SEDs) of XBs that are well sampled in both wavelength and time. Here we focus on the evolution of the jet in their broadband spectra. Some of the most densely sampled broadband SEDs of a neutron star transient (IGR J00291+5934) are used to constrain the optically thick-thin break in the jet spectrum. For the black hole transient XTE J1550-564, infrared - X-ray correlations, evolution of broadband spectraand timing signatures indicate that synchrotron emission from the jet likely dominates the X-ray power law at low luminosities during the hard state outburst decline.

AB - Most accretion-powered relativistic jet sources in our Galaxy are transient X-ray binaries (XBs). Efforts to coordinate multiwavelength observations of these objects have improved dramatically over the last decade. Now the challenge is to interpret broadband spectral energy distributions (SEDs) of XBs that are well sampled in both wavelength and time. Here we focus on the evolution of the jet in their broadband spectra. Some of the most densely sampled broadband SEDs of a neutron star transient (IGR J00291+5934) are used to constrain the optically thick-thin break in the jet spectrum. For the black hole transient XTE J1550-564, infrared - X-ray correlations, evolution of broadband spectraand timing signatures indicate that synchrotron emission from the jet likely dominates the X-ray power law at low luminosities during the hard state outburst decline.

KW - accretion

KW - accretion discs

KW - x-rays

KW - binaries

KW - ism

KW - jets and outflows

U2 - 10.1017/S1743921310016285

DO - 10.1017/S1743921310016285

M3 - Article

VL - 6

SP - 317

EP - 318

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

ER -

Isolating the jet in broadband spectra of XBs

Abstract

Keywords

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