722 citations · 1.3k across the 13 of their papers we have counts for
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Touchstone Stars: Highlights from the Cool Stars 18 Splinter Session
Andrew W. Mann, Adam Kraus, Tabetha Boyajian +11
We present a summary of the splinter session on "touchstone stars" -- stars with directly measured parameters -- that was organized as part of the Cool Stars 18 conference. We disc…
The G+M eclipsing binary V530 Orionis: A stringent test of magnetic stellar evolution models for low-mass stars
G. Torres, C. H. Sandberg Lacy, K. Pavlovski +4
We report extensive photometric and spectroscopic observations of the 6.1-day period, G+M-type detached double-lined eclipsing binary V530 Ori, an important new benchmark system fo…
Updating the Dartmouth Stellar Evolution Model Grid: Pre-Main-Sequence Models & Magnetic Fields
Gregory A. Feiden, Jaquille Jones, Brian Chaboyer
We present the current status of an effort to create an updated grid of low-mass stellar evolution mass tracks and isochrones computed using the Dartmouth stellar evolution code. E…
BANYAN. IV. Fundamental parameters of low-mass star candidates in nearby young stellar kinematic groups - Isochronal Age determination using Magnetic evolutionary models
Lison Malo, René Doyon, Gregory A. Feiden +5
Based on high resolution optical spectra obtained with ESPaDOnS at CFHT, we determine fundamental parameters (\Teff, R, \Lbol, \logg\ and metallicity) for 59 candidate members of n…
Empirical Tests of Pre-Main-Sequence Stellar Evolution Models with Eclipsing Binaries
Keivan G. Stassun, Gregory A. Feiden, Guillermo Torres
We examine the performance of standard PMS stellar evolution models against the accurately measured properties of a benchmark sample of 26 PMS stars in 13 EB systems. We provide a…
Revised age for CM Draconis and WD 1633+572: Toward a resolution of model-observation radius discrepancies
Gregory A. Feiden, Brian Chaboyer
We report an age revision for the low-mass detached eclipsing binary CM Draconis and its common proper motion companion, WD 1633+572. An age of 8.5 3.5 Gyr is found by combin…