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Spatial Distribution of AlO in a High-mass Protostar Candidate Orion Source I
2019
Astrophysical Journal Letters
High-temperature molecular gas containing metallic elements is potentially a good probe to trace the kinematics/ dynamics of circumstellar disks, and its presence in circumstellar disks around young stellar objects (YSOs) may also give some insights into formation processes of high-temperature meteoritic components formed in the Sun's protoplanetary disk. The Orion Kleimann-Low (KL) region is the most famous and nearest massive star formation site, and has been extensively studied since the
doi:10.3847/2041-8213/ab1653
fatcat:nnvvssdzyrbznegryr4nekea4i