Volume 558, October 2013
|Number of page(s)||18|
|Section||Interstellar and circumstellar matter|
|Published online||16 October 2013|
Figures A.1 to A.6 show comparisons between the observations and the best-fit models for the larger sample of sources. Table A.1 provides the observation identification numbers for all Herschel observations included in this paper.
Comparison of outflow and baseline subtracted observations for L1527 (black) with the best-fit model (red). The green error bar and scaling factors are the same as in Fig. 6.
|Open with DEXTER|
Observation identification numbers.
© ESO, 2013
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