2011Astronomy and AstrophysicsOpen access

Chromosphere of K giant stars

P. Bério, T. Merle, Mathieu Thévenin, Dominique Bonneau, D. Mourard, O. Chesneau, O. Delaa, R. Ligi, N. Nardetto, K. Perraut, Bruno Pichon, P. Stee, I. Tallon–Bosc, J. M. Clausse, A. Spang, Harold A. McAlister, Theo A. ten Brummelaar, J. Sturmann, L. Sturmann, N. Turner, C. Farrington, P. J. Goldfinger

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Abstract

Context. Interferometers provide accurate diameter measurements of stars by analyzing both the continuum and the lines formed in photospheres and chromospheres. Tests of the geometrical extent of the chromospheres are therefore possible by comparing the estimated radius in the continuum of the photosphere and the estimated radii in chromospheric lines.

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Context. Interferometers provide accurate diameter measurements of stars by analyzing both the continuum and the lines formed in photospheres and chromospheres. Tests of the geometrical extent of the chromospheres are therefore possible by comparing the estimated radius in the continuum of the photosphere and the estimated radii in chromospheric lines.

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Available abstract

Context. Interferometers provide accurate diameter measurements of stars by analyzing both the continuum and the lines formed in photospheres and chromospheres. Tests of the geometrical extent of the chromospheres are therefore possible by comparing the estimated radius in the continuum of the photosphere and the estimated radii in chromospheric lines.

Key concepts: Chromosphere, Astrophysics, Photosphere, Physics, Stars, RADIUS, Stellar atmosphere, Astronomy

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