Issue |
A&A
Volume 576, April 2015
|
|
---|---|---|
Article Number | A5 | |
Number of page(s) | 10 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201425484 | |
Published online | 13 March 2015 |
Online material
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Fig. 3
Observed lines of aGg′-(CH2OH)2 toward the protostar NGC 1333 IRAS2A (in black). The best-fit model for aGg′-(CH2OH)2 (see Table 2) is shown as red solid lines. The contributions of the CH3OCHO and CH2OHCHO lines are indicated with green and blue lines. The model including aGg′-(CH2OH)2, CH2OHCHO, and CH3OCHO can be seen as red dotted lines. |
Open with DEXTER |
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Fig. 4
Observed lines of CH3OCHO toward the protostar NGC 1333 IRAS2A (in black). The best-fit model for CH3OCHO (see Table 2) is shown as red lines. |
Open with DEXTER |
CH2OHCHO, aGg′-(CH2OH)2 and CH3OCHO transitions observed toward NGC 1333 IRAS2A.
© ESO, 2015
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