Skip to main content
SearchLoginLogin or Signup

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
·

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.

The full text of this article is only available in PDF format:

Comments
0
comment
No comments here