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20112022
most citedWeakened magnetic braking as the origin of anomalously rapid rotation in old field stars

417 citations · 2.6k across the 34 of their papers we have counts for

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Showing 2016Show all

5 papers · 1 filter

astro-ph.SR2016★ 88 cited

Constraining the efficiency of angular momentum transport with asteroseismology of red giants: the effect of stellar mass

P. Eggenberger, N. Lagarde, A. Miglio +12

Context: Constraints on the internal rotation of red giants are now available thanks to asteroseismic observations. Preliminary comparisons with rotating stellar models indicate th…

astro-ph.SR2016★ 2 cited

Constraining stellar physics from red-giant stars in binaries - stellar rotation, mixing processes and stellar activity

P. G. Beck, T. Kallinger, K. Pavlovski +10

The unparalleled photometric data obtained by NASA's Kepler Space Telescope has led to an improved understanding of stellar structure and evolution - in particular for solar-like o…

astro-ph.SR2016★ 66 cited

Photospheric and chromospheric magnetic activity of seismic solar analogs. Observational inputs on the solar/stellar connection from Kepler and Hermes

D. Salabert, R. A. Garcia, P. G. Beck +8

We identify a set of 18 solar analogs among the seismic sample of solar-like stars observed by the Kepler satellite rotating between 10 and 40 days. This set is constructed using t…

astro-ph.SR2016★ 53 cited

Magnetic variability in the young solar analog KIC 10644253: Observations from the Kepler satellite and the HERMES spectrograph

D. Salabert, C. Regulo, R. A. Garcia +12

The continuous photometric observations collected by the Kepler satellite over 4 years provide a whelm of data with an unequalled quantity and quality for the study of stellar evol…

astro-ph.SR2016★ 417 cited

Weakened magnetic braking as the origin of anomalously rapid rotation in old field stars

Jennifer L. van Saders, Tugdual Ceillier, Travis S. Metcalfe +5

A knowledge of stellar ages is crucial for our understanding of many astrophysical phenomena, and yet ages can be difficult to determine. As they become older, stars lose mass and…