@article{fa4504451784436082edb5d2ae1f6dbe,
title = "Asteroseismic detection of latitudinal differential rotation in 13 Sun-like stars",
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{\textquoteright} equators rotate approximately twice as fast as their midlatitudes. The latitudinal shear inferred from asteroseismology is much larger than predictions from numerical simulations.",
author = "O. Benomar and M. Bazot and Nielsen, {M. B.} and L. Gizon and T. Sekii and M. Takata and H. Hotta and S. Hanasoge and Sreenivasan, {K. R.} and J. Christensen-Dalsgaard",
note = "Funding Information: This work is supported by NYUAD institute grant G1502. Research funding from the German Aerospace Center (Grant 50OO1501) and the Max Planck Society (PLATO Science) is acknowledged. Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (grant DNRF106). The research was supported by the ASTERISK project (ASTERoseismic Investigations with SONG and Kepler) funded by the European Research Council (grant agreement 267864). Funding for the Kepler mission is provided by the NASA Science Mission directorate. Publisher Copyright: 2017 {\textcopyright} The Authors, some rights reserved.",
year = "2018",
month = sep,
day = "21",
doi = "10.1126/science.aao6571",
language = "English (US)",
volume = "361",
pages = "1231--1234",
journal = "Science",
issn = "0036-8075",
publisher = "American Association for the Advancement of Science",
number = "6408",
}