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Time-Domain Photometry of Protostars at Far-Infrared and Submillimeter Wavelengths

Published onMay 31, 2019
Time-Domain Photometry of Protostars at Far-Infrared and Submillimeter Wavelengths
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Abstract

The majority of the main-sequence mass of a star is assembled in the protostellar phase, where a forming star is embedded in an infalling envelope and encircled by a protoplanetary disk. We discuss the progress that would be enabled with far-infrared and submillimeter programs to probe protostellar accretion variability in the nearest kiloparsec.

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