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MIAO-ALMA: Shocks and Protostellar Outflows in 70 μm Dark Clumps with L/M < 1 L⊙/M⊙

  • Authors: Shuting Lin, Siyi Feng, Junzhi Wang, Shanghuo Li, Dan Miao, Zhi-Yu Zhang, Sheng-Yuan Liu, Nami Sakai, Fengwei Xu, Hauyu Baobab Liu, Henrik Beuther, Di Li, Qizhou Zhang, Tie Liu, Patricio Sanhueza, Olli Sipilä, Ken'ichi Tatematsu, Jaime E. Pineda, Xing Lu

Shuting Lin et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 5.

(a) Core mass versus outflow mass, with the bivariate Gaussian kernel density estimate (KDE) shown as blue contour lines. (b) Core mass versus outflow velocity, with a bivariate KDE. The core mass is adopted from Feng (2026, in preparation). In both panels, each orange dot represents an individual outflow, while the gray lines show the linear fits. The Spearman’s rank correlation coefficient (ρ), the corresponding p-value, and the best-fit parameters are indicated in each panel.

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