A break in the gas and dust surface density of the disc around the T Tauri star IM Lup
Olja Pani\'c, Michiel R. Hogerheijde, David Wilner, Chunhua Qi

TL;DR
This study investigates the distribution of gas and dust in the IM Lup protoplanetary disc, revealing a significant density drop near 400 AU and suggesting a high gas-to-dust ratio beyond this radius.
Contribution
It provides a detailed comparison of gas and dust distributions in the IM Lup disc, highlighting a density discontinuity and refining the disc model with observational data.
Findings
Gas disc extends to 900 AU, dust to 400 AU
Density drops sharply near 400 AU
Gas-to-dust ratio is at least 100 beyond 400 AU
Abstract
We study the distribution and physical properties of molecular gas in the disc around the T Tauri star IM Lup on scales close to 200 AU. We investigate how well the gas and dust distributions compare and work towards a unified disc model that can explain both gas and dust emission. 12CO, 13CO, and C18O J=2-1 line emission, as well as the dust continuum at 1.3 mm, is observed at 1.8" resolution towards IM Lup using the Submillimeter Array. A detailed disc model based on the dust emission is tested against these observations with the aid of a molecular excitation and radiative transfer code. Apparent discrepancies between the gas and dust distribution are investigated by adopting simple modifications to the existing model. The disc is seen at an inclination of 54+/-3 degrees and is in Keplerian rotation around a 0.8-1.6 Msun star. The outer disc radius traced by molecular gas emission is…
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