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How do stars gain their mass? A JCMT/SCUBA 2 transient survey of protostars in nearby star forming regions

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Figure

Fig. 1.— The SCUBA-2 850The marks show the location of Class 0, Class I, and flat spectrum protostars, as identified and classified by Dunham et al
Fig. 2.— The distribution of 342 peaks with 850ness above 0.125 Jy/beam for all eight regions in our survey (yel-low)
Fig. 3.— The expected fraction of time that a given theoreti-cal model returns an amplitude variation greater than a specificamount as a function of the time lag between observations
Protostars and disks identified with bright sub-mm peaksTABLE 2a

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