Observational Signatures of Tightly Wound Spirals Driven by Buoyancy Resonances in Protoplanetary Disks

<p>These are simulated CO data cubes presented in &quot;Observational Signatures of Tightly Wound Spirals Driven by Buoyancy Resonances in Protoplanetary Disks&quot; by Bae, Teague and Zhu. They represent simulated 12CO and 13CO ALMA observations using the standard model (see Section 3.1.1 of the paper), with three different planet masses (0.5, 1, and 2 Jupiter-mass) and five different disk inclination values (5, 15, 30, 45, and 60 degrees).</p>