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  Asteroseismic detection of latitudinal differential rotation in 13 Sun-like stars

Benomar, O., Bazot, M., Nielsen, M. B., Gizon, L., Sekii, T., Takata, M., et al. (2018). Asteroseismic detection of latitudinal differential rotation in 13 Sun-like stars. Science, 361(6408), 1231-1234. doi:10.1126/science.aao6571.

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 Creators:
Benomar, O., Author
Bazot, M., Author
Nielsen, M. B., Author
Gizon, Laurent1, Author           
Sekii, T., Author
Takata, M., Author
Hotta, H., Author
Hanasoge, S., Author
Sreenivasan, K. R., Author
Christensen-Dalsgaard, J., Author
Affiliations:
1Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832287              

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 Abstract: The differentially rotating outer layers of stars are thought to play a role in driving their magnetic activity, but the underlying mechanisms that generate and sustain differential rotation are poorly understood. We report the measurement using asteroseismology of latitudinal differential rotation in the convection zones of 40 Sun-like stars. For the most significant detections, the stars’ equators rotate approximately twice as fast as their midlatitudes. The latitudinal shear inferred from asteroseismology is much larger than predictions from numerical simulations.

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 Dates: 2019-03-132018
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1126/science.aao6571
 Degree: -

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Title: Science
  Other : Science
Source Genre: Journal
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Publ. Info: Washington, D.C. : American Association for the Advancement of Science
Pages: - Volume / Issue: 361 (6408) Sequence Number: - Start / End Page: 1231 - 1234 Identifier: ISSN: 0036-8075
CoNE: https://pure.mpg.de/cone/journals/resource/991042748276600_1