July 12, 2017 Poster Open Access

Ferrero, L.V.; Cappa, C.E.; Gomez, M.

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    <subfield code="a">&lt;p&gt;We present a multi-frequency study of HH 137 and HH 138 using Gemini images and APEX molecular line&lt;br&gt;
data, as well as Spitzer images. Several 2.12 micron knots linked to HH137 are identified in the Gemini image. 12^CO(3-2),&lt;br&gt;
13^CO(3-2), and C18^O(3-2) line data reveal the molecular counterpart of HH 137. Spitzer combined images suggest the&lt;br&gt;
location of the exciting source of HH 137, almost coincident with a high-density molecular clump detected in C18^O. We&lt;br&gt;
derive the main physical parameters of the molecular clump and the molecular outflow, and propose a simple scenario for the&lt;br&gt;
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