Issue |
A&A
Volume 527, March 2011
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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
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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Open with DEXTER |
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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Open with DEXTER |
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. |
|
Open with DEXTER |
© ESO, 2011
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