Ferrero, L.V.
Cappa, C.E.
Gomez, M.
2017-07-12
<p>We present a multi-frequency study of HH 137 and HH 138 using Gemini images and APEX molecular line<br>
data, as well as Spitzer images. Several 2.12 micron knots linked to HH137 are identified in the Gemini image. 12^CO(3-2),<br>
13^CO(3-2), and C18^O(3-2) line data reveal the molecular counterpart of HH 137. Spitzer combined images suggest the<br>
location of the exciting source of HH 137, almost coincident with a high-density molecular clump detected in C18^O. We<br>
derive the main physical parameters of the molecular clump and the molecular outflow, and propose a simple scenario for the<br>
whole complex.</p>
https://doi.org/10.5281/zenodo.826357
oai:zenodo.org:826357
Zenodo
https://zenodo.org/communities/starformation2017
https://doi.org/10.5281/zenodo.826356
info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
HH137 and 138: discovering new knots and a molecular outflow with Gemini and APEX
info:eu-repo/semantics/conferencePoster