MATISSE L-band data on HD 100453 inner disk supports misalignment and requires asymmetric structures beyond simple symmetric models.
D.1.Temperature gradient model best-fit MCMC chains, forR out =10 AU, after removing burn-in to the combined PIONIER, GRA VITY & MATISSE datasets
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The complex inner disk of the Herbig Ae star HD 100453 with VLTI/MATISSE
MATISSE L-band data on HD 100453 inner disk supports misalignment and requires asymmetric structures beyond simple symmetric models.