Volume 532, August 2011
|Number of page(s)||22|
|Section||Interstellar and circumstellar matter|
|Published online||21 July 2011|
Parameters of the models that fit the H2 observations of HH320AB and HH321AB (separated by the double horizontal line).
Parameters of the models that fit the H2 observations of the SiO knot.
Predicted integrated intensities of the o-H2O lines to be targeted by the HIFI and PACS receivers of the Herschel telescope.
Predicted integrated intensities of the p-H2O lines to be targeted by the HIFI and PACS receivers of the Herschel telescope.
© ESO, 2011
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