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Q/W-band Observations toward Starless Cores in Orion (QWOSCO). I. Overview, Isotopologues, Isomers, and Complex Organics

  • Authors: Shih-Ying Hsu, Xunchuan Liu, Sheng-Yuan Liu, Tie Liu, Naomi Hirano, Mika Juvela, Kee-Tae Kim, Chin-Fei Lee, Shanghuo Li, Sheng-Jun Lin, Sheng-Li Qin, Dipen Sahu, Ken'ichi Tatematsu, Fengwei Xu, L. Viktor Tóth

Shih-Ying Hsu et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 4.

The scatter plots of the CH3OH and CH3CHO column densities in starless cores from different clouds. The data of Taurus and Perseus clouds were adopted from S. Scibelli & Y. Shirley (2020) and S. Scibelli et al. (2024), respectively. The r and ρ represent the Pearson and Spearman correlation coefficients, respectively. In panel (a), the ﹩{r}^{{\prime} }﹩ and ﹩{\rho }^{{\prime} }﹩ are the coefficients excluding the outlier illustrated by the white color.

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