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Showing 1 to 1 of 1 for “"visibility modeling"”.
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Circumstellar Structure Properties of Young Stellar Objects: Envelopes, Bipolar Outflows, and Disks
… by CARMA at 1.3 mm and 2.7 mm continuum. Through visibility modeling to fit the two wavelength continuum data simultaneously, we found that the dust opacity spectral index of Class 0 YSOs is around unity, which implies that dust grains have significantly grown already at the earliest stage. In …