activity
19992014
most citedYREC: The Yale Rotating Stellar Evolution Code

230 citations · 412 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2014★ 28 cited

Modeling Convective Core Overshoot and Diffusion in Procyon Constrained by Asteroseismic Data

D. B. Guenther, P. Demarque, M Gruberbauer

We compare evolved stellar models, which match Procyons mass and position in the HR diagram, to current ground-based asteroseismic observations. Diffusion of helium and metals alon…

astro-ph.SR2012★ 10 cited

Delta Scuti stars in the Praesepe cluster observed by the MOST satellite

M. Breger, M. Hareter, Markus Endl +8

The Praesepe cluster contains a number of Delta Sct and Gamma Dor pulsators. Asteroseismology of cluster stars is simplified by the common distance, age and stellar abundances. Sin…

astro-ph.SR2011★ 24 cited

New SPB stars in the field of the young open cluster NGC 2244 discovered by the MOST photometric satellite

D. Gruber, H. Saio, R. Kuschnig +9

During two weeks of nearly continuous optical photometry of the young open cluster NGC 2244 obtained by the MOST satellite, we discovered two new SPB stars, GSC 00154-00785 and GSC…

astro-ph.SR2011★ 18 cited

Pulsational analysis of V 588 Mon and V 589 Mon observed with the MOST and CoRoT satellites

Konstanze Zwintz, Thomas Kallinger, David B. Guenther +8

The two pulsating pre-main sequence (PMS) stars V 588 Mon and V 589 Mon were observed by CoRoT for 23.4 days in March 2008 during the Short Run SRa01 and in 2004 and 2006 by MOST f…

astro-ph.SR2010★ 14 cited

Photometric variability of the Herbig Ae star HD 37806

S. M. Rucinski, K. Zwintz, M. Hareter +7

The more massive counterparts of T Tauri stars, Herbig Ae/Be stars, are known to vary in a complex way with no variability mechanism clearly identified. We attempt to characterize…

astro-ph2007★ 230 cited

YREC: The Yale Rotating Stellar Evolution Code

P. Demarque, D. B. Guenther, L. H. Li +2

The stellar evolution code YREC is outlined with emphasis on its applications to helio- and asteroseismology. The procedure for calculating calibrated solar and stellar models is d…