Brian Chaboyer
0000-0003-3096-4161
Dartmouth College
93 papers found
Refreshing results…
On the Use of Field RR Lyrae as Galactic Probes. I. The Oosterhoff Dichotomy Based on Fundamental Variables
Infrared K-band Photometry of Field RR Lyrae Variable Stars
Are the Double-mode Bulge RR Lyrae Stars with Identical Period Ratios the Relic of a Disrupted Stellar System?
Erratum: “High-resolution Spectroscopic Abundances of Red Giant Branch Stars in NGC 6584 and NGC 7099” (2018, ApJ, 856, 130)
On a New Method to Estimate the Distance, Reddening, and Metallicity of RR Lyrae Stars Using Optical/Near-infrared (B, V, I, J, H, K) Mean Magnitudes: ω Centauri as a First Test Case
Classically and Asteroseismically Constrained 1D Stellar Evolution Models of α Centauri A and B Using Empirical Mixing Length Calibrations
High-resolution Spectroscopic Abundances of Red Giant Branch Stars in NGC 6584 and NGC 7099
Not All Stars Are the Sun: Empirical Calibration of the Mixing Length for Metal-poor Stars Using One-dimensional Stellar Evolution Models
High-resolution Spectroscopic Abundances of Red Giant Branch Stars in NGC 6681
Absolute Ages and Distances of 22 GCs Using Monte Carlo Main-sequence Fitting
A Differential Abundance Analysis of Very Metal-poor Stars
Testing Metal-poor Stellar Models and Isochrones withHSTParallaxes of Metal-poor Stars
Investigating the Consistency of Stellar Evolution Models With Globular Cluster Observations via the Red Giant Branch Bump
Revised age for CM Draconis and WD 1633+572
Magnetic Inhibition of Convection and the Fundamental Properties of Low-Mass Stars. Ii. Fully Convective Main-Sequence Stars
The Acs Survey of Globular Clusters. Xiii. Photometric Calibration in Comparison With Stetson Standards
BVI photometry and the red giant branch luminosity function of M15
Magnetic Inhibition of Convection and the Fundamental Properties of Low-Mass Stars. I. Stars With a Radiative Core
The Rr Lyrae Variables and Horizontal Branch of Ngc 6656 (M22),
Do Magnetic Fields Actually Inflate Low-Mass Stars?
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