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 following magnetic heartbeats of late-type stars via high-contrast coronal X-rays. Goal is to provide fundamental observational constraints for contemporary and future studies of underlying magnetic Dynamo, whose internal workings remain elusive. The Sun's high-energy modulations play important "Space Weather" role in our heliosphere, as do stellar counterparts for their exoplanets. 3-year time series (joint with HST) is proposed for promising new candidates Xi Boo (G8V+K4) and 70 Oph (K0V+K5V), adding four more dwarfs to the three in current "Cycles." Key question involves origin of diverging branches in rotational period vs. cycle duration, where Sun's iconic 11-yr example sits in the middle, possibly in a transitional state. |
Remarks: This is a Preference: 1st observation could be scheduled early-Apr 2020, and 2nd observation in early-Sep 2020 (both windows at unconstrained pitch angles); repeat in subsequent 2 Cycles. |
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