Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence That Disks Can Be Optically Thick at 3 mm
Accurate disk mass measurements are necessary to constrain disk evolution and the timescale of planet formation, but such measurements are difficult to make and are very dependent on assumptions. Here, we look at the assumption that the disk is optically thin at radio wavelengths and the effect of t...
Main Authors: | Z. Xin, C. C. Espaillat, A. M. Rilinger, Á. Ribas, E. Macías |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2022-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/aca52b |
Similar Items
-
Determining Dust Properties in Protoplanetary Disks: SED-derived Masses and Settling with ALMA
by: Anneliese M. Rilinger, et al.
Published: (2023-01-01) -
JWST Detects Neon Line Variability in a Protoplanetary Disk
by: C. C. Espaillat, et al.
Published: (2023-01-01) -
A Magnetically Driven Disk Wind in the Inner Disk of PDS 70
by: Justyn Campbell-White, et al.
Published: (2023-01-01) -
Ionization of protoplanetary disks by galactic cosmic rays, solar protons, and supernova remnants
by: Ryuho Kataoka, et al.
Published: (2017-03-01) -
Observational Signatures of Planets in Protoplanetary Disks: Planet-induced Line Broadening in Gaps
by: Ruobing Dong, et al.
Published: (2019-01-01)