Wide field CO J = 3  →  2 mapping of the Serpens cloud core

O. Dionatos; B. Nisini; C. Codella; T. Giannini

doi:10.1051/0004-6361/200913839

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Volume 523 (November-December 2010)

A&A, 523 (2010) A29

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Fig. 5

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Magnification of the high-velocity gas of Area B from Fig. 1 superimposed on an IRAC band 2 (upper panel) and MIPS band 1 (lower panel) images (in grayscale). Contour levels are as in Fig. 1.

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