C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: Chandra has been tracking coronal activity cycles of late-type stars via high-contrast soft X-rays, jointly with HST to capture UV tracers. Objective is to provide fundamental observational constraints for contemporary and future studies of the underlying magnetic dynamo, whose inner workings remain elusive. The Sun's high-energy modulations play an important "Space Weather" role in our heliosphere, as do stellar counterparts for their exoplanets. 3-year time-domain campaign (joint with HST) is proposed for iconic Alpha Centauri, already followed by HRC-I since 2006. The Alpha Cen field also is rich in serendipitous sources, including flaring red dwarfs and several possibly cycling F-K stars. |
Remarks: Clarification: the spacing indicated in the Observing Time tab is meant to indicate two observations per year, about six months apart. |
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