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The Powering Source and Origin of the Quadrupolar Molecular Outflow in L723

  • Authors: Naomi Hirano, Saeko S. Hayashi, Tomofumi Umemoto, and Nobuharu Ukita

Hirano et al. 1998 The Astrophysical Journal 504 334.

  • Provider: AAS Journals

Caption: Fig. 6.

(a) Comparison of the blueshifted CO outflow (VLSR = 3.02–7.07 km s−1; contours) and the blueshifted CS J = 3–2 component (VLSR = 10.1–10.6 km s−1; gray scale). The contours of the CO and CS map are drawn in the same manner as in Figs. 3 and 2, respectively. The positions of VLA 1, VLA 2, HH 82, and HH 84 are denoted by crosses. (b) Comparison of the redshifted CO outflow (VLSR = 11.93–20.03 km s−1; contours) and the CS J = 3–2 component of VLSR = 11.1–11.6 km s−1 (gray scale). The contours of the CO map are every 1.82 Jy km s−1 beam−1 (1.5 σ) with the lowest contours of 3.65 Jy km s−1 beam−1 (3 σ). The contours of the CS map are drawn in the same manner as in Fig. 2.

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