Tying the Geometrical Traits of Massive Young Stellar Objects and Their Disks to a Potential Evolutionary Sequence Using Infrared Observations (2021)
Attributed to:
A Programme of Research in Astronomical Theory, Astronomical Observations and Planetary and Solar System Science
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/ac1741
Publication URI: http://dx.doi.org/10.3847/1538-4357/ac1741
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1