X-ray emission from the fast rotating A7 star Altair

Physics

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Scientific paper

We propose to observe the low activity star Altair with the Chandra LETGS. With a spectral type of A7, the very fast rotator Altair is the earliest, magnetically active, single late-type star detected by ROSAT and Einstein. Its X-ray luminosity is low and the activity level as expressed by the L_X/L_bol ratio is the lowest measured in any nearby star. Being located at a distance of only 5 pc, Altair is a unique target to study the X-ray properties of late A-type stars in greater detail. The proposed 100 ks observation will enable us to investigate the cool corona of a star with a very shallow convection zone in this spectral range. We expect to measure rotationally broadened stellar emission lines in the X-ray regime for the first time.

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