Free Access
Issue
A&A
Volume 527, March 2011
Article Number A39
Number of page(s) 17
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201015012
Published online 21 January 2011

Online material

thumbnail Fig. 4

Velocity position diagrams of the H2CO(30,3−20,2), HDCO(41,4−31,3), D2CO(40,4−30,3), and C18O(3 − 2) lines along the declination axis at Δα = 0′′. The molecule is indicated in each panel. The C18O(3 − 2) data are from Liseau et al. (2010). The vertical scale in each panel indicates the declination offset and the horizontal scale is the vLSR velocity. The intensity scale in all four panels is Tmb.

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thumbnail Fig. 5

Ortho H2CO(31,2−21,1) and (31,2−21,1) spectra at declination offsets  − 30″ (bottom, D-peak), 0″ (middle) and  + 30″ (top, P1). The offsets are relative the center position in Fig. 1. The  spectra (in colour) have been scaled up with a factor of 10 and appear much more noisy.

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thumbnail Fig. 8

SO(56−45) and (65−54) map spectra toward the ρ Oph A cloud. The  spectra (in colour) have been multiplied with a factor of 5. Scales as in Fig. 2.

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© ESO, 2011

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