Sub-millimeter light curves of IRC+10216 and o Ceti show the same periods as their optical variability, and IRC+10216's 850-micron peak lags its optical peak by about 540 days.
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The Sub-mm Variability of IRC+10216 and $o$ Ceti
Sub-millimeter light curves of IRC+10216 and o Ceti show the same periods as their optical variability, and IRC+10216's 850-micron peak lags its optical peak by about 540 days.