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Stars, Gas, and Star Formation of Distant Post-starburst Galaxies

  • Authors: Po-Feng Wu, 柏鋒 吳, Rachel Bezanson, Francesco D'Eugenio, Anna R. Gallazzi, Jenny E. Greene, Michael V. Maseda, Katherine A. Suess, Arjen van der Wel

Po-Feng Wu et al 2023 The Astrophysical Journal 955 .

  • Provider: AAS Journals

Caption: Figure 4.

The moment 0 maps of CO(2-1) and best-fit Gaussian models. Contours increase every 3σ, starting from 3σ, where σ is measured from the central 3′ of the residual maps. The beam sizes are plotted at the lower-left corners. All three CO(2-1) emissions can be modeled by a single Gaussian component, with no clear sign of disturbed morphology or outflow under the current resolution.

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