Coronal Mass Ejections As a Mechanism for Producing IR Variability in Debris Disks
classification
🌌 astro-ph.SR
keywords
coronaldisksejectionsinfraredmassmechanismobservationsactivity
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Motivated by recent observations of short-timescale variations in the infrared emission of circumstellar disks, we propose that coronal mass ejections can remove dust grains on timescales as short as a few days. Continuous monitoring of stellar activity, coupled to infrared observations, can place meaningful constraints on the proposed mechanism.
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