A dust-evolution model predicts AB Aurigae b's circumplanetary disk is too faint at 1.3 mm to have been detected, unless extinction-corrected planet properties are used, in which case the non-detection implies a dust-poor inflow.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Predictions of Dust Continuum Emission from a Potential Circumplanetary Disk: A Case Study of the Planet Candidate AB Aurigae b
A dust-evolution model predicts AB Aurigae b's circumplanetary disk is too faint at 1.3 mm to have been detected, unless extinction-corrected planet properties are used, in which case the non-detection implies a dust-poor inflow.