US EditionMulti-Wavelength Dust Characterization of the HL Tau Disk and Implications for Planet Formation - Astrobiology
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Multi-Wavelength Dust Characterization of the HL Tau Disk and Implications for Planet Formation - Astrobiology
We present a comprehensive analysis of the HL Tau dust disk by modeling its intensity profiles across six wavelengths (0.45 to 7.9 mm) with a resolution of 0.05 arcsec (∼7 au). Using a Markov Chain Monte Carlo (MCMC) approach, we constrain key dust properties including temperature, surface density, maximum grain size, composition, filling factor, and […] The post Multi-Wavelength Dust Characterization of the HL Tau Disk and Implications for Plan…
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