Jets from X-ray binaries

Rob Fender

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arXiv · astro-ph/0303339

Jets from X-ray binaries

Rob Fender

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Abstract

Relativistic outflows, or `Jets', represent one of the most obvious, important and yet poorly-explained phenomena associated with accreting relativistic objects, including X-ray binaries. In the past decade we have observed highly relativistic flows, the resultant in-situ particle acceleration in the ISM, and begun to unearth the subtleties of the accretion -- outflow coupling on timescales from seconds to years. In this chapter I shall attempt, subjectively, to describe the state of research into jets from X-ray binaries as it stands at the beginning of 2003.

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BibTeX RIS

Rob Fender. 2003-08-28. Jets from X-ray binaries. https://arxiv.org/abs/astro-ph/0303339

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