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arXiv · astro-ph/0603003

A magnetically collimated jet from an evolved star

W. H. T. Vlemmings·P. J. Diamond·H. Imai
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Abstract

Planetary nebulae often have asymmetric shapes, which could arise due to collimated jets from evolved stars before evolution to the planetary nebula phase. The source of jet collimation in these stars is unknown. Magnetic fields are thought to collimate outflows that are observed in many other astrophysical sources, such as active galactic nuclei and proto-stars, although hitherto there are no direct observations of both the magnetic field direction and strength in any collimated jet. Theoretical models have shown that magnetic fields could also be the dominant source of collimation of jet in evolved stars. Here we report measurements of the polarization of water vapour masers that trace the precessing jet emanating from the asymptotic giant branch star W43A at 2.6 kpc from the Sun, which is undergoing rapid evolution into a planetary nebula. The masers occur in two clusters at opposing tips of the jets, ~1,000 AU from the star. We find direct evidence that the magnetic field is collimating the jet.

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W. H. T. Vlemmings, P. J. Diamond, H. Imai. 2006-02-28. A magnetically collimated jet from an evolved star. https://doi.org/10.1038/nature04466

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