First observations of stellar coronal structure - The coronae of AR Lacertae

Astronomy and Astrophysics – Astronomy

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Coronal Loops, Eclipsing Binary Stars, Flare Stars, Radio Sources (Astronomy), Stellar Coronas, X Ray Sources, Chromosphere, Heao 2, Light Curve, Magnetic Flux, Stellar Luminosity, Stellar Magnetic Fields, Stellar Spectra, Stellar Structure, Subgiant Stars, Ultraviolet Spectra

Scientific paper

In connection with the present investigation, X-ray, radio, and ultraviolet observations of AR Lacertae over one orbital cycle have been obtained. The X-ray light curve shows a deep primary minimum and a broad, shallow secondary minimum. The quiescent corona of the G2 IV component is small and asymmetric. This corona extends some 0.02 stellar radii above the photosphere; the leading, spotted hemisphere is brighter in X-rays than the trailing hemisphere. The K0 IV component has two coronal components. The extended, presumably hotter component extends to one stellar radius above the photosphere and exhibits a brighter leading hemisphere. There is an inner coronal component which is small relative to the stellar radius, but the lack of coverage past mid-eclipse severely limits the possibility to deduce the nature of this component. The UV observations also imply a nonuniform surface distribution of plage regions.

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