Multiple relativistic outbursts of GRS 1915+105: radio emission and internal shocks

Details Multiple relativistic outbursts of GRS 1915+105: radio emission and internal shocks Multiple relativistic outbursts of GRS 1915+105: radio emission and internal shocks

2005-08-10

arxiv.org/abs/astro-ph/0508230v1

Mon.Not.Roy.Astron.Soc.363:867-881,2005

Astronomy and Astrophysics

Astrophysics

18 pages, 14 figures, accepted for publication in MNRAS. For higher-resolution versions of Figures 3, 5, and 12, see http://

Scientific paper

10.1111/j.1365-2966.2005.09488.x

We present 5-GHz MERLIN radio images of the microquasar GRS 1915+105 during two separate outbursts in 2001 March and 2001 July, following the evolution of the jet components as they move outwards from the core of the system. Proper motions constrain the intrinsic jet speed to be >0.57c, but the uncertainty in the source distance prevents an accurate determination of the jet speed. No deceleration is observed in the jet components out to an angular separation of about 300mas. Linear polarisation is observed in the approaching jet component, with a gradual rotation in position angle and a decreasing fractional polarisation with time. Our data lend support to the internal shock model whereby the jet velocity increases leading to internal shocks in the pre-existing outflow before the jet switches off. The compact nuclear jet is seen to re-establish itself within two days, and is visible as core emission at all epochs. The energetics of the source are calculated for the possible range of distances; a minimum power of 1-10 per cent of the Eddington luminosity is required to launch the jet.

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