ALMA Band 9 CO(6--5) Reveals a Warm Ring Structure Associated with the Embedded Protostar in the Cold Dense Core MC 27/L1521F
arXiv:2602.12661 · doi:10.3847/2041-8213/ae47ec
Abstract
Infall and outflows, coupled with magnetic fields, rapidly structure the gas around newborn protostars. Shocks from interacting components encode the temperature and density distribution, offering a direct probe of the earliest evolution history. However, interferometric observations characterizing warm envelopes using high-excitation lines remain scarce. We present ALMA Band 9 observations of the Taurus dense core MC 27/L1521F, which hosts a Class 0 protostar, targeting the CO(=6-5) line at an angular resolution of 2\arcsec\ (300 au). We detect an off-centered ring-like structure with a diameter of 1000 au that was not identifiable in previous low- CO data, where emission close to the systemic velocity is strongly affected by optical depth. The ring shows a typical peak brightness temperature of 3 K at our resolution. Excitation considerations indicate that the detected CO(=6-5) emission likely arises from relatively warm ( K) and dense ( cm) gas embedded within the surrounding cold, dense core. The morphology and kinematics suggest an energetic and localized shock-heating event, potentially linked to dynamical gas--magnetic-field interactions in the earliest protostellar phase. Our results demonstrate that high- CO observations provide a powerful new window on warm and dense gas components, enabling a more direct view of the physical processes operating at the onset of star formation.
12 pages, 5 figures, accepted for publication in ApJL
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