ALMA Measurements of Circumstellar Material in the GQ Lup System
Meredith A. MacGregor, David J. Wilner, Ian Czekala, Sean M. Andrews,, Y. Sophia Dai, Gregory J. Herczeg, Kaitlin M. Kratter, Adam L. Kraus, Luca, Ricci, Leonardo Testi

TL;DR
This study uses ALMA observations to characterize the dust and gas disk around GQ Lup A, constrain the star's mass and disk orientation, and set upper limits on any circumplanetary disk around GQ Lup b, informing formation theories.
Contribution
First detailed ALMA imaging of the GQ Lup system's circumstellar disk, providing constraints on the star's mass, disk geometry, and limits on circumplanetary material around the companion.
Findings
The circumprimary dust disk has a FWHM of 59±12 AU.
The gas disk extends to a radius of approximately 46.5 AU.
No significant circumplanetary disk detected around GQ Lup b, with an upper mass limit of 0.04 Earth masses.
Abstract
We present ALMA observations of the GQ Lup system, a young Sun-like star with a substellar mass companion in a wide-separation orbit. These observations of 870 m continuum and CO J=3-2 line emission with beam size ( AU) resolve the disk of dust and gas surrounding the primary star, GQ Lup A, and provide deep limits on any circumplanetary disk surrounding the companion, GQ Lup b. The circumprimary dust disk is compact with a FWHM of AU, while the gas has a larger extent with a characteristic radius of AU. By forward-modeling the velocity field of the circumprimary disk based on the CO emission, we constrain the mass of GQ Lup A to be , where is a known distance, and determine that we view the disk at an inclination angle of and a position angle of $346^\circ…
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