FAUST I. The hot corino at the heart of the prototypical Class I protostar L1551 IRS5
E. Bianchi, C. J. Chandler, C. Ceccarelli, C. Codella, N. Sakai, A., L\'opez-Sepulcre, L. T. Maud, G. Moellenbrock, B. Svoboda, Y. Watanabe, T., Sakai, F. M\'enard, Y. Aikawa, F. Alves, N. Balucani, M. Bouvier, P. Caselli,, E. Caux, S. Charnley, S. Choudhury, M. De Simone

TL;DR
This paper reports the discovery of a hot corino in a Class I protostar, L1551 IRS5, revealing chemical similarities with earlier Class 0 hot corinos and providing insights into early planetary system chemistry.
Contribution
The first detection of a hot corino in a Class I protostar using ALMA, expanding understanding of hot corino evolution from Class 0 to I phases.
Findings
Detected methanol, methyl formate, and ethanol lines in L1551 IRS5.
Constrained gas temperature (~100 K) and density (≥1.5×10^8 cm^-3).
Found chemical abundances similar to Class 0 hot corinos.
Abstract
The study of hot corinos in Solar-like protostars has been so far mostly limited to the Class 0 phase, hampering our understanding of their origin and evolution. In addition, recent evidence suggests that planet formation starts already during Class I phase, which, therefore, represents a crucial step in the future planetary system chemical composition. Hence, the study of hot corinos in Class I protostars has become of paramount importance. Here we report the discovery of a hot corino towards the prototypical Class I protostar L1551 IRS5, obtained within the ALMA Large Program FAUST. We detected several lines from methanol and its isopotologues (CHOH and CHDOH), methyl formate and ethanol. Lines are bright toward the north component of the IRS5 binary system, and a possible second hot corino may be associated with the south component. The methanol lines…
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