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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. 4.

CO J = 1–0 maps of blueshifted (VLSR = −1.04–11.12 km s−1; blue contours) and redshifted (VLSR = 11.93–24.08 km s−1; red contours) emission taken by the NMA superposed on the CS J = 3–2 integrated intensity map taken by the 45 m telescope (green shaded). The contours of the CO J = 1–0 maps are drawn every 1.7 Jy km s−1 beam−1 (1 σ) from the 3.4 Jy km s−1 beam−1 (2 σ) level. The contours of the CS J = 3–2 map are drawn in the same manner as in Fig. 1b. The positions of two radio continuum sources (VLA 1 and VLA 2) and HH objects identified by Vrba et al. (1986) (HH 82 and HH 84) are indicated by crosses.

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