activity
20102020
most citedThe Aarhus Red Giants Challenge I: Stellar structures in the red giant branch phase

56 citations · 141 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2020★ 13 cited

Asteroseismic sensitivity to internal rotation along the red-giant branch

F. Ahlborn, E. P. Bellinger, S. Hekker +2

Transport of angular momentum in stellar interiors is currently not well understood. Asteroseismology can provide us with estimates of internal rotation of stars and thereby advanc…

astro-ph.SR2020★ 35 cited

The Aarhus red giants challenge II. Stellar oscillations in the red giant branch phase

J. Christensen-Dalsgaard, V. Silva Aguirre, S. Cassisi +23

Context. The large quantity of high-quality asteroseismic data that obtained from space-based photometric missions and the accuracy of the resulting frequencies motivate a careful…

astro-ph.SR2020★ 14 cited

Mirror principle and the red-giant bump: the battle of entropy in low-mass stars

S. Hekker, G. C. Angelou, Y. Elsworth +1

The evolution of low-mass stars into red giants is still poorly understood. During this evolution the core of the star contracts and, simultaneously, the envelope expands -- a proc…

astro-ph.SR2019★ 56 cited

The Aarhus Red Giants Challenge I: Stellar structures in the red giant branch phase

V. Silva Aguirre, J. Christensen-Dalsgaard, S. Cassisi +23

(Abridged). We introduce the Aarhus Red Giants Challenge, a series of detailed comparisons between widely used stellar evolution and oscillation codes aiming at establishing the mi…

astro-ph.SR2012★ 19 cited

Cyanogen in NGC 1851 RGB and AGB Stars: Quadrimodal Distributions

S. W. Campbell, D. Yong, E. C. Wylie-de Boer +7

The Galactic globular cluster NGC 1851 has raised much interest since HST photometry revealed that it hosts a double subgiant branch. Here we report on our homogeneous study into t…

astro-ph.SR2010★ 1 cited

Observational Constraints for Thermohaline Mixing

G. C. Angelou, J. C. Lattanzio, R. P. Church +1

We provide a brief review of thermohaline physics and why it is a candidate extra mixing mechanism during the red giant branch (RGB). We discuss how thermohaline mixing (also calle…