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• W3100225937 abstract "We introduce new analysis methods for studying the star cluster formation processes in Orion A, especially examining the scenario of a cloud-cloud collision. We utilize the CARMA-NRO Orion survey $^{13}$CO (1-0) data to compare molecular gas to the properties of YSOs from the SDSS III IN-SYNC survey. We show that the increase of $v_{rm 13CO} - v_{rm YSO}$ and $Sigma$ scatter of older YSOs can be signals of cloud-cloud collision. SOFIA-upGREAT 158$mu$m [CII] archival data toward the northern part of Orion A are also compared to the $^{13}$CO data to test whether the position and velocity offsets between the emission from these two transitions resemble those predicted by a cloud-cloud collision model. We find that the northern part of Orion A, including regions ONC-OMC-1, OMC-2, OMC-3 and OMC-4, shows qualitative agreements with the cloud-cloud collision scenario, while in one of the southern regions, NGC1999, there is no indication of such a process in causing the birth of new stars. On the other hand, another southern cluster, L1641N, shows slight tendencies of cloud-cloud collision. Overall, our results support the cloud-cloud collision process as being an important mechanism for star cluster formation in Orion A." @default.
• W3100225937 created "2020-11-23" @default.
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• W3100225937 date "2020-05-25" @default.
• W3100225937 modified "2023-10-01" @default.
• W3100225937 title "Star cluster formation in Orion A" @default.
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• W3100225937 doi "https://doi.org/10.1093/pasj/psaa035" @default.
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