We present angular diameters of the Hyades giants, γ, δ1, , and θ1 Tau from interferometric measurements with the CHARA Array. Our errors in the limb-darkened angular diameters for these stars are all less than 2%, and in combination with additional observable quantities, we determine the effective temperatures, linear radii, and absolute luminosities for each of these stars. Additionally, stellar masses are inferred from model isochrones to determine the surface gravities. These data show that a new calibration of effective temperatures with errors well under 100 K is now possible from interferometric angular diameters of stars
Using the longest baselinesof theCHARAArray,wehavemeasured the angular diameter of theG5Vsubdwarf Ca...
Using the longest baselines of the CHARA Array, we have measured the angular diameter of the G5 V su...
We have determined the angular diameters of two metal-poor stars, HD 122563 and Gmb 1830, using CHAR...
We present angular diameters of the Hyades giants, γ, δ1, ε, and θ1 Tau from interferometric measure...
Using Georgia State University’s Center for High Angular Resolution Astronomy Array interferometer, ...
We present interferometric angular diameter measurements of 21 low-mass, K- and M-dwarfs made with t...
We have executed a survey of nearby, main-sequence A-, F-, and G-type stars with the CHARA Array, su...
We present interferometric observations of 25 spectral type-B stars that were made with the Precisio...
We have executed a survey of nearby, main-sequence A-, F-, and G-type stars with the CHARA Array, su...
We have executed a survey of nearby, main-sequence A-, F-, and G-type stars with the CHARA Array, su...
For the main part of this dissertation, I have executed a survey of nearby, main sequence A, F, and ...
Based on CHARA Array measurements, we present the angular diameters of 23 nearby, main-sequence star...
We have measured the angular diameters for a sample of 24 exoplanet host stars using Georgia State U...
We present interferometric observations of six O-type stars that were made with the Precision Astron...
Based on CHARA Array measurements, we present the angular diameters of 23 nearby, main-sequence star...
Using the longest baselinesof theCHARAArray,wehavemeasured the angular diameter of theG5Vsubdwarf Ca...
Using the longest baselines of the CHARA Array, we have measured the angular diameter of the G5 V su...
We have determined the angular diameters of two metal-poor stars, HD 122563 and Gmb 1830, using CHAR...
We present angular diameters of the Hyades giants, γ, δ1, ε, and θ1 Tau from interferometric measure...
Using Georgia State University’s Center for High Angular Resolution Astronomy Array interferometer, ...
We present interferometric angular diameter measurements of 21 low-mass, K- and M-dwarfs made with t...
We have executed a survey of nearby, main-sequence A-, F-, and G-type stars with the CHARA Array, su...
We present interferometric observations of 25 spectral type-B stars that were made with the Precisio...
We have executed a survey of nearby, main-sequence A-, F-, and G-type stars with the CHARA Array, su...
We have executed a survey of nearby, main-sequence A-, F-, and G-type stars with the CHARA Array, su...
For the main part of this dissertation, I have executed a survey of nearby, main sequence A, F, and ...
Based on CHARA Array measurements, we present the angular diameters of 23 nearby, main-sequence star...
We have measured the angular diameters for a sample of 24 exoplanet host stars using Georgia State U...
We present interferometric observations of six O-type stars that were made with the Precision Astron...
Based on CHARA Array measurements, we present the angular diameters of 23 nearby, main-sequence star...
Using the longest baselinesof theCHARAArray,wehavemeasured the angular diameter of theG5Vsubdwarf Ca...
Using the longest baselines of the CHARA Array, we have measured the angular diameter of the G5 V su...
We have determined the angular diameters of two metal-poor stars, HD 122563 and Gmb 1830, using CHAR...