Add to ORKGWe have measured the angular diameters for a sample of 24 exoplanet host stars using Georgia State University’s CHARA Array interferometer. We use these improved angular diameters together with Hipparcos parallax measure-ments to derive linear radii and to estimate the stars ’ evolutionary states
We present the results of long-baseline optical interferometry observations using the Precision Astr...
We have measured the angular diameter of the transiting extrasolar planet host star HD 189733 using ...
We measured the angular diameter of the exoplanet host star ι Dra with Georgia State University’s Ce...
Until the last decade or so, our entire knowledge of planets around Sun-like stars consisted of thos...
Using Georgia State University’s Center for High Angular Resolution Astronomy Array interferometer, ...
We present interferometric observations of 25 spectral type-B stars that were made with the Precisio...
Until the last decade or so, our entire knowledge of planets around Sun-like stars consisted of thos...
We present angular diameters of the Hyades giants, γ, δ1, , and θ1 Tau from interferometric measurem...
We have been using the CHARA Interferometric Array on Mount Wilson over the course of the last 4 yea...
International audienceOver the last few years, a new generation of long baseline interferometers has...
Context. Accurate stellar parameters are needed in numerous domains of astrophysics. The position of...
International audienceContext. Accurate stellar parameters are needed in numerous domains of astroph...
We present angular diameters of the Hyades giants, γ, δ1, ε, and θ1 Tau from interferometric measure...
We present the three dimensional orbits of eight double-lined spectroscopic binaries with longer orb...
We present the results of long-baseline optical interferometry observations using the Precision Astr...
We present the results of long-baseline optical interferometry observations using the Precision Astr...
We have measured the angular diameter of the transiting extrasolar planet host star HD 189733 using ...
We measured the angular diameter of the exoplanet host star ι Dra with Georgia State University’s Ce...
Until the last decade or so, our entire knowledge of planets around Sun-like stars consisted of thos...
Using Georgia State University’s Center for High Angular Resolution Astronomy Array interferometer, ...
We present interferometric observations of 25 spectral type-B stars that were made with the Precisio...
Until the last decade or so, our entire knowledge of planets around Sun-like stars consisted of thos...
We present angular diameters of the Hyades giants, γ, δ1, , and θ1 Tau from interferometric measurem...
We have been using the CHARA Interferometric Array on Mount Wilson over the course of the last 4 yea...
International audienceOver the last few years, a new generation of long baseline interferometers has...
Context. Accurate stellar parameters are needed in numerous domains of astrophysics. The position of...
International audienceContext. Accurate stellar parameters are needed in numerous domains of astroph...
We present angular diameters of the Hyades giants, γ, δ1, ε, and θ1 Tau from interferometric measure...
We present the three dimensional orbits of eight double-lined spectroscopic binaries with longer orb...
We present the results of long-baseline optical interferometry observations using the Precision Astr...
We present the results of long-baseline optical interferometry observations using the Precision Astr...
We have measured the angular diameter of the transiting extrasolar planet host star HD 189733 using ...
We measured the angular diameter of the exoplanet host star ι Dra with Georgia State University’s Ce...