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- W4386875210 abstract "According to the structures traced by $^{13}$CO spectral lines within the $^{12}$CO molecular clouds (MCs), we investigate the contributions of their internal gas motions and relative motions to the total velocity dispersions of $^{12}$CO MCs. Our samples of 2851 $^{12}$CO MCs harbor a total of 9556 individual $^{13}$CO structures, among which 1848 MCs ($sim$ 65$%$) have one individual $^{13}$CO structure and the other 1003 MCs ($sim$ 35$%$) have multiple $^{13}$CO structures. We find that the contribution of the relative motion between $^{13}$CO structures ($sigma_{rm ^{13}CO, re}$) is larger than that from their internal gas motion ($sigma_{rm ^{13}CO, in}$) in $sim$ 62$%$ of 1003 MCs in the `multiple' regime. In addition, we find the $sigma_{rm ^{13}CO, re}$ tends to increase with the total velocity dispersion($sigma_{rm ^{12}CO, tot}$) in our samples, especially for the MCs having multiple $^{13}$CO structures. This result provides a manifestation of the macro-turbulent within MCs, which gradually becomes the dominant way to store the kinetic energy along with the development of MC scales." @default.
- W4386875210 created "2023-09-20" @default.
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- W4386875210 date "2023-09-16" @default.
- W4386875210 modified "2023-10-18" @default.
- W4386875210 title "Understanding the Kinetic Energy deposition within Molecular Clouds" @default.
- W4386875210 doi "https://doi.org/10.48550/arxiv.2309.08998" @default.
- W4386875210 hasPublicationYear "2023" @default.
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