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Formation of Counterrotating Stellar Disks in the S0 Galaxy PGC 66551

  • Authors: Liuze Long, Min Bao, Qiusheng Gu, Yanmei Chen, Shiying Lu, Yuren Zhou

Liuze Long et al 2026 The Astrophysical Journal 1012 .

  • Provider: AAS Journals

Caption: Figure 3.

CO distribution of PGC 66551. (a) and (b) The integrated intensity in Jy beam–1 km s−1 and velocity of CO, using a threshold of 2.7 mJy (∼5σrms). The beam size is shown at the bottom-left corner. (c) Spatial distribution of SFE. The black dashed lines in panels (a) and (b) are the same as Figure 1. The black ellipse in panel (c) presents the new beam size after the convolution.

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