Revealing the gas properties of the most typical planet-forming disks
Year: 2024
Type: article
Abstract: Planets are formed from the gas and dust in disks around young stars, both of which will benefit from the Wideband Sensitivity Upgrade. However, the largest limitation to analyzing the emission from these disks will continue to be the limited angular resolution and image reconstruction methods. In this talk, I will present how visibility-based techniques can efficiently recover the gas morphology and brightness temperature in compact and faint disks, where image-based techniques are unable to operate. These techniques will be crucial to optimize the recovery of information of the improved spectral scan capabilities. These results are part of Kurtovic \& Pinilla
Author: Kurtovic, Nicolas
Institution: Max Planck Institute for Extraterrestrial Physics
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W6949116065
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