A sensitive search for soft X-rays from Arcturus and Procyon

Astronomy and Astrophysics – Astronomy

Scientific paper

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Giant Stars, Stellar Atmospheres, Stellar Mass Ejection, X Ray Astronomy, X Ray Stars, Coronas, Mass Transfer, Proportional Counters, Rocket Flight

Scientific paper

Sensitive X-ray observations have been obtained of alpha Boo and alpha CMi using rocket-borne large area proportional counters. No flux was detected from either star, yielding limits on intrinsic luminosity in the 75-2000 eV band (6-165 A) as stringent as 10 to the 28-th power ergs per sec depending upon assumed coronal temperature. These are at least an order of magnitude better limits than previously reported values. Upper limits are also set on a mass loss rate of three billionths solar mass per year and on an emission measure of less than 3 times 10 to the 53-rd power per cu cm. If these stars are typical, then giants and subgiants cannot be responsible for a significant fraction of the soft component of the diffuse X-ray background.

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