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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. 5.

Comparison of the interferometric CO map (blue and red contours) and the single‐dish CO J = 1–0 map observed with the 45 m telescope by Hayashi et al. (1991; blue and red shaded). The contours of the interferometric map are drawn in the same manner as in Fig. 4. The velocity intervals of the single‐dish map are from −5 to 8 km s−1 for the blueshifted (blue shaded; lowest 3, step 1 K km s−1) and from 13 to 26 km s−1 for the redshifted (red shaded; lowest 2, step 1 K km s−1) components. Crosses denote the positions of VLA 1 and VLA 2.

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