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A magnetically collimated jet from an evolved star

Overview of attention for article published in Nature, March 2006
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Title
A magnetically collimated jet from an evolved star
Published in
Nature, March 2006
DOI 10.1038/nature04466
Pubmed ID
Authors

Wouter H. T. Vlemmings, Philip J. Diamond, Hiroshi Imai

Abstract

Planetary nebulae often have asymmetric shapes, even though their progenitor stars were symmetric; this structure could be the result of collimated jets from the evolved stars before they enter the planetary nebula phase. Theoretical models have shown that magnetic fields could be the dominant source of jet-collimation in evolved stars, just as these fields are thought to collimate outflows in other astrophysical sources, such as active galactic nuclei and proto-stars. But hitherto there have been no direct observations of both the magnetic field direction and strength in any collimated jet. 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 a distance of 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, approximately 1,000 au from the star. We conclude from the data that the magnetic field is indeed collimating the jet.

Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 23 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
United Kingdom 2 9%
United States 1 4%
China 1 4%
Unknown 19 83%

Demographic breakdown

Readers by professional status Count As %
Researcher 7 30%
Professor > Associate Professor 4 17%
Student > Ph. D. Student 4 17%
Professor 3 13%
Other 1 4%
Other 0 0%
Unknown 4 17%
Readers by discipline Count As %
Physics and Astronomy 15 65%
Chemistry 2 9%
Sports and Recreations 1 4%
Biochemistry, Genetics and Molecular Biology 1 4%
Unknown 4 17%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 3. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 09 April 2024.
All research outputs
#8,527,033
of 25,378,162 outputs
Outputs from Nature
#70,633
of 97,719 outputs
Outputs of similar age
#30,830
of 92,012 outputs
Outputs of similar age from Nature
#350
of 466 outputs
Altmetric has tracked 25,378,162 research outputs across all sources so far. This one is in the 43rd percentile – i.e., 43% of other outputs scored the same or lower than it.
So far Altmetric has tracked 97,719 research outputs from this source. They typically receive a lot more attention than average, with a mean Attention Score of 102.4. This one is in the 11th percentile – i.e., 11% of its peers scored the same or lower than it.
Older research outputs will score higher simply because they've had more time to accumulate mentions. To account for age we can compare this Altmetric Attention Score to the 92,012 tracked outputs that were published within six weeks on either side of this one in any source. This one is in the 12th percentile – i.e., 12% of its contemporaries scored the same or lower than it.
We're also able to compare this research output to 466 others from the same source and published within six weeks on either side of this one. This one is in the 10th percentile – i.e., 10% of its contemporaries scored the same or lower than it.