Poster Open Access
Ferrero, L.V.; Cappa, C.E.; Gomez, M.
{ "description": "<p>We present a multi-frequency study of HH 137 and HH 138 using Gemini images and APEX molecular line<br>\ndata, as well as Spitzer images. Several 2.12 micron knots linked to HH137 are identified in the Gemini image. 12^CO(3-2),<br>\n13^CO(3-2), and C18^O(3-2) line data reveal the molecular counterpart of HH 137. Spitzer combined images suggest the<br>\nlocation of the exciting source of HH 137, almost coincident with a high-density molecular clump detected in C18^O. We<br>\nderive the main physical parameters of the molecular clump and the molecular outflow, and propose a simple scenario for the<br>\nwhole complex.</p>", "license": "https://creativecommons.org/licenses/by/4.0/legalcode", "creator": [ { "affiliation": "OAC, Cordoba, Argentina", "@type": "Person", "name": "Ferrero, L.V." }, { "affiliation": "CONICET, Argentina", "@type": "Person", "name": "Cappa, C.E." }, { "affiliation": "OAC, Cordoba, Argentina", "@type": "Person", "name": "Gomez, M." } ], "url": "https://zenodo.org/record/826357", "datePublished": "2017-07-12", "@context": "https://schema.org/", "identifier": "https://doi.org/10.5281/zenodo.826357", "@id": "https://doi.org/10.5281/zenodo.826357", "@type": "CreativeWork", "name": "HH137 and 138: discovering new knots and a molecular outflow with Gemini and APEX" }
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