Deuterated water in the solar-type protostars NGC 1333 IRAS 4A and IRAS 4B

A. Coutens; C. Vastel; S. Cabrit; C. Codella; L. E. Kristensen; C. Ceccarelli; E. F. van Dishoeck; A. C. A. Boogert; S. Bottinelli; A. Castets; E. Caux; C. Comito; K. Demyk; F. Herpin; B. Lefloch; C. McCoey; J. C. Mottram; B. Parise; V. Taquet; F. F. S.  van der Tak; R. Visser; U. A. Yıldız

doi:10.1051/0004-6361/201322400

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Volume 560 (December 2013)

A&A, 560 (2013) A39

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Fig. 10

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Comparison of the line profiles of the CO 6–5 transition (in red), the HDO 1_1,1–0_0,0 transition (in black, intensities multiplied by 150), and the H₂O 1_1,1–0_0,0 transition (in green, intensities multiplied by 15) towards IRAS 4A.

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