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Open AccessJournal ArticleDOI

Interferometry and asteroseismology: The radius of τ Cet

TLDR
In this article, the radius of the nearby star τ Cet has been determined from interferometry using the VINCI instrument on VLTI using the siderostats.
Abstract
We have determined from interferometry the radius of the nearby star τ Cet, using recent observations with the VINCI instrument on VLTI using the siderostats. The limb-darkened disk diameter is determined, with an unprecedented internal precision of 0.5%, to be 1.971 ± 0.009(int.) ± 0.05(ext.) mas, corresponding to a physical radius of 0.773 ± 0.004(int.) ± 0.02(ext.) R� . With this determination τ Cet becomes a prime target for asteroseismic campaigns to determine its internal structure, and thereby test stellar evolution theory. We discuss implications for asteroseismology and present predictions for oscillation properties.

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Journal ArticleDOI

A search for debris discs around stars with giant planets

TL;DR: In this article, the primordial disc mass was used to explain why stars that do not have debris should preferentially only have distant planets, i.e., few stars possess both inner planets and a disc, indicating that these phenomena either are not connected or are mutually exclusive.
Journal ArticleDOI

Integrated optics for astronomical interferometry - VI. Coupling the light of the VLTI in K band

TL;DR: In this paper, the authors used the commissioning data obtained with the dedicated K-band integrated optics two-telescope beam combiner which now replaces the fiber coupler MONA in the VLTI/VINCI instrument to prove that integrated optics is not only a good concept for astronomical interferometry but also a working technique with high performance.
Journal ArticleDOI

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)

TL;DR: In this article, the authors compare solar UV spectra with archival STIS spectra from the Hubble Space Telescope of α Cen A (G2 V, V = 3.5) to understand the roles of acoustic and magnetic mechanisms in heating the outer atmospheres of Sun-like stars.
Journal ArticleDOI

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

TL;DR: In this article, the authors used the Sydney University Stellar Interferometer (SUSI) to measure the angular diameter of β Hydri, a nearby G2 subgiant the mean density of which was recently measured with high precision using asteroseismology.
Journal ArticleDOI

First observations with an H-band integrated optics beam combiner at the VLTI

TL;DR: In this article, the authors reported results obtained with the Very Large Telescope Interferometer Commissioning Instrument (VLTI-VINCI) where the fiber interferometric coupler MONA was temporarily replaced by an integrated optics beam com- biner (IONIC).
References
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Journal ArticleDOI

Updated Opal Opacities

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Journal ArticleDOI

Solar models with helium and heavy-element diffusion

TL;DR: In this article, the effects on neutrino fluxes of each change in the input physics are evaluated separately by constructing a series of solar models with one additional improvement added at each stage.
Journal ArticleDOI

Spectral Irradiance Calibration in the Infrared. X. A Self-Consistent Radiometric All-Sky Network of Absolutely Calibrated Stellar Spectra

TL;DR: In this article, the authors start from six absolutely calibrated continuous stellar spectra from 1.2 to 35?m for K0, K1.5, K3, K5, and M0 giants, and normalize each template by photometry for the individual stars using published and/or newly secured near and mid-infrared photometry obtained through fully characterized, absolutely calibrated, combinations of filter passband, detector radiance response, and mean terrestrial atmospheric transmission.
Book

Solar Interior and Atmosphere

TL;DR: In this article, observational data derived from the world's largest solar telescopes are correlated with theoretical discussions in nuclear and atomic physics by contributors representing a wide range of interests in solar research, focusing both on processes occurring at the interior of the Sun and on complicated features observed at its surface.
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