| Issue |
A&A
Volume 528, April 2011
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 1 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201015475e | |
| Published online | 16 March 2011 | |
Extended emission of D2H+ in a prestellar core⋆ (Corrigendum)
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
e-mail: bparise@mpifr-bonn.mpg.de
Key words: astrochemistry / line: identification / stars: formation / ISM: molecules / errata, addenda
An error occurred during the production process in Figs. 7, 8, and 9, leading to a corrupted linestyle for the curves corresponding to x(CO) =10-5. The corrected figures are published below.
 |
Fig. 7 Time evolution of the chemistry for T = 12 K. The different colors stand for different densities: n = 104 (blue), 105 (green), 106 cm-3 (red). The thick lines represent the o/p H2 ratio. The thin lines represent the p-D2H+/o-H2D+ ratio. The different line styles stand for different CO abundances: complete depletion (full), xCO = 10-6 (dash), xCO = 10-5 (dash-dot). |
 |
Fig. 8 Steady-state ortho-to-para ratio of H2. |
 |
Fig. 9 Chemical model predictions of the p-D2H+/o-H2D+ ratio (same convention as previous figures), at steady state. The thick decreasing lines show the ratio derived from the non-LTE analysis of the observations, in the assumption of different densities and different o/p-H2 ratios (same curves as presented in Fig. 6 but with the same linestyle for both o-p H2 ratios). |
© ESO, 2011
All Figures
|
Fig. 7 Time evolution of the chemistry for T = 12 K. The different colors stand for different densities: n = 104 (blue), 105 (green), 106 cm-3 (red). The thick lines represent the o/p H2 ratio. The thin lines represent the p-D2H+/o-H2D+ ratio. The different line styles stand for different CO abundances: complete depletion (full), xCO = 10-6 (dash), xCO = 10-5 (dash-dot). |
| In the text | |
|
Fig. 8 Steady-state ortho-to-para ratio of H2. |
| In the text | |
|
Fig. 9 Chemical model predictions of the p-D2H+/o-H2D+ ratio (same convention as previous figures), at steady state. The thick decreasing lines show the ratio derived from the non-LTE analysis of the observations, in the assumption of different densities and different o/p-H2 ratios (same curves as presented in Fig. 6 but with the same linestyle for both o-p H2 ratios). |
| In the text | |
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