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Detection of a Disk Surrounding the Variably Accreting Young Star HBC722

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arxiv 2009.08019 v1 pith:OQNOEAEV submitted 2020-09-17 astro-ph.GA

Xi Yek (Zach) , Michael M. Dunham , Héctor G. Arce , Tyler L. Bourke , Xuepeng Chen , Joel D. Green , Agnes Kospal , Steven N. Longmore This is my paper
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keywords hbc722detectiondiskaccretingalmaburstcalculatecircumstellar
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We present new ALMA 233 GHz continuum observations of the FU Orionis Object HBC722. With these data we detect HBC722 at millimeter wavelengths for the first time, use this detection to calculate a circumstellar disk mass of 0.024 solar masses, and discuss implications for the burst triggering mechanism.

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    A Gaussian process trained on simulated skin wave experiments predicts stress and pre-stretch from two surface wave speeds with R2=0.957, but the full method lacks in vivo validation.

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