Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 4.

PV diagrams of SiO (2–1) narrow-line-width, spatially extended SiO (2–1) components in G12.95–0.25, G14.18–0.23, and G14.23–0.18, extracted along the directions of the orange arrows shown in the velocity-integrated intensity maps (Figure 1). Black contours represent the narrow SiO (2–1) component, starting at 3σ and increasing in steps of 4σ, with 1σ = 0.0041 Jy beam−1. The black horizontal dashed line indicates the systemic velocity of the clump.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse