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• W3033705833 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." @default.
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• W3033705833 date "2019-03-18" @default.
• W3033705833 modified "2023-09-27" @default.
• W3033705833 title "Time-Domain Photometry of Protostars at Far-Infrared and Submillimeter Wavelengths" @default.
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