Seeing the unseen: a method to detect unresolved rings in protoplanetary disks
Chiara E. Scardoni, Richard A. Booth, Cathie J. Clarke, Giovanni P., Rosotti, Alvaro Ribas

TL;DR
This paper introduces a novel method to detect unresolved, optically thick dust rings in protoplanetary disks by analyzing azimuthal brightness variations, aiding in understanding planet formation processes.
Contribution
The authors propose an innovative observational technique using brightness peaks at the minor axis to identify unresolved rings and infer their properties in protoplanetary disks.
Findings
Brightness peaks indicate unresolved rings in inclined disks.
Azimuthal brightness variations reveal ring optical properties.
Method is applicable to ALMA observations of protoplanetary disks.
Abstract
While high resolution ALMA observations reveal a wealth of substructure in protoplanetary discs, they remain incapable of resolving the types of small scale dust structures predicted, for example, by numerical simulations of the streaming instability. In this Letter, we propose a method to find evidence for unresolved, optically thick dusty rings in protoplanetary disks. We demonstrate that, in presence of unresolved rings, the brightness of an inclined disc exhibits a distinctive emission peak at the minor axis. Furthermore, the azimuthal brightness depends on both the geometry of the rings and the dust optical properties; we can therefore use the azimuthal brightness variations to both detect unresolved rings and probe their properties. By analyzing the azimuthal brightness in the test-case of ring-like substructures formed by streaming instability, we show that the resulting peak is…
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