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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. 1.

Integrated intensity maps of CS emission taken with the NRO 45 m telescope. (a) The CS J = 2–1 emission integrated over 9.1–12.6 km s−1. The lowest contour level is 1.12 K km s−1 (3 σ), and the contour spacing is 0.56 K km s−1 (1.5 σ). The positions of VLA 1 and VLA 2 are indicated by crosses. (b) The CS J = 3–2 emission. The velocity range is the same as that in (a). The lowest contour level is 0.56 K km s−1 (3 σ), and the contour spacing is 0.28 K km s−1 (1.5 σ).

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