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Models of the Hydrodynamic Histories of Post-AGB Stars. I. Multiflow Shaping of OH 231.8+04.2

  • Authors: Bruce Balick, Adam Frank, Baowei Liu, and Martín Huarte-Espinosa

2017 The Astrophysical Journal 843 108.

  • Provider: AAS Journals

Caption: Figure 1.

Images of OH231 in optical light (left) and 12CO (right) taken from the literature. Left: an overlay of optical and near-IR images of OH231 obtained from the Hubble Legacy Archive. North is up. The white circle provides an image scale. Right: spatial distribution and axial Doppler speeds of 12CO lines from OH231 obtained at the Plateau de Bure interferometer and republished with permission (CO panel source: a Web document entitled “From the AGB to the PN phase with the Plateau de Bure Interferometer“ posted as a PDF file by A. Castro-Carrizo with J.M. Winters and R. Neri, c. 1998, with no public URL. These CO results were subsequently reformatted and republished by A+01). The upper (lower) row shows the images and kinematic results for the 12CO(1–0) (12CO(2–1)) line.

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