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Cited article:

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Asteroseismic Analysis of α Cen B: Preliminary Tests of Effects of Rotation and Interior Magnetic Field in the Solar-like Star

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The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation

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The Complementary Roles of Interferometry and Asteroseismology in Determining the Mass of Solar‐Type Stars

O. L. Creevey, M. J. P. F. G. Monteiro, T. S. Metcalfe, et al.
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Interferometric observations of the multiple stellar systemδ Velorum

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Models of   Centauri A and B with and without seismic constraints: time dependence of the mixing-length parameter

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The radius and mass of the subgiant star β Hyi from interferometry and asteroseismology

J. R. North, J. Davis, T. R. Bedding, M. J. Ireland, A. P. Jacob, J. O'Byrne, S. M. Owens, J. G. Robertson, W. J. Tango and P. G. Tuthill
Monthly Notices of the Royal Astronomical Society: Letters 380 (1) L80 (2007)
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Probing turbulence with seismic observations of α Centauri

C. W. Straka, P. Demarque and F. J. Robinson
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Solar‐like Oscillations in the Metal‐poor Subgiant ν Indi: Constraining the Mass and Age Using Asteroseismology

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Establishing Visible Interferometer System Responses: Resolved and Unresolved Calibrators

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The Effective Temperature Scale of FGK Stars. I. Determination of Temperatures and Angular Diameters with the Infrared Flux Method

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Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs

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Stellar Lyα Emission Lines in the Hubble Space Telescope Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and Astrospheres

Brian E. Wood, Seth Redfield, Jeffrey L. Linsky, Hans‐Reinhard Muller and Gary P. Zank
The Astrophysical Journal Supplement Series 159 (1) 118 (2005)
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Squared Visibility Estimators: Calibrating Biases to Reach Very High Dynamic Range

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The Astrophysical Journal 626 (2) 1138 (2005)
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VLTI/VINCI diameter constraints on the evolutionary status ofδEri,ξHya,ηBoo

F. Thévenin, P. Kervella, B. Pichon, et al.
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A Comparison of the Outer Atmosphere of the “Flat Activity” Star τ Ceti (G8 V) with the Sun (G2 V) and α Centauri A (G2 V)

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The Astrophysical Journal 609 (1) 392 (2004)
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A Preliminary Seismic Analysis of 51 Pegasi: Large and Small Spacings from Standard Models

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Cooler and Bigger than Previously Thought? Planetary Host Stellar Parameters from the Infrared Flux Method

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Cepheid distances from infrared long-baseline interferometry

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The interferometric diameter and internal structure of Sirius A

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