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Modelling oscillations in the jet emission from microquasar GRS 1915+105

Record type: Article

The variability in the infrared to millimetre emission from microquasar GRS 1915+105 is believed to be dominated by the system's relativistic jet. In this paper we develop a time-dependent version of the jet emission model of Blandford & Königl and apply it to the oscillations in the infrared and millimetre emission from GRS 1915+105 observed recently by Fender & Pooley. The resulting model provides a reasonable description of the observed flux oscillations from GRS 1915+105. From a fit of the observed time lag between the flux peaks in the infrared and millimetre emission together with the flux normalization, we were able to determine the model parameters for the GRS 1915+105 jet. We find that to achieve the observed flux levels with the model requires an unphysically large electron density within the jet. We therefore conclude that the Blandford & Königl model cannot explain these observations, either because it does not provide the correct description of the emission from microquasar jets, or because the observed emission variations do not originate in the jet.

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Citation

Collins, R.S., Kaiser, C.R. and Cox, S.J. (2003) Modelling oscillations in the jet emission from microquasar GRS 1915+105 Monthly Notices of the Royal Astronomical Society, 338, (2), pp. 331-339. (doi:10.1046/j.1365-8711.2003.06100.x).

More information

Published date: 2003
Keywords: non-thermal radiation mechanisms, close binaries, GRS 1915+105, ISM, jets, outflows, infrared, radio continuum, stars

Identifiers

Local EPrints ID: 22373
URI: http://eprints.soton.ac.uk/id/eprint/22373
ISSN: 0035-8711
PURE UUID: 20be4fa2-eee5-43f4-8b34-8792aa0930a1

Catalogue record

Date deposited: 24 Mar 2006
Last modified: 17 Jul 2017 16:22

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