Poster Open Access

HH137 and 138: discovering new knots and a molecular outflow with Gemini and APEX

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


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  <identifier identifierType="DOI">10.5281/zenodo.826357</identifier>
  <creators>
    <creator>
      <creatorName>Ferrero, L.V.</creatorName>
      <givenName>L.V.</givenName>
      <familyName>Ferrero</familyName>
      <affiliation>OAC, Cordoba, Argentina</affiliation>
    </creator>
    <creator>
      <creatorName>Cappa, C.E.</creatorName>
      <givenName>C.E.</givenName>
      <familyName>Cappa</familyName>
      <affiliation>CONICET, Argentina</affiliation>
    </creator>
    <creator>
      <creatorName>Gomez, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Gomez</familyName>
      <affiliation>OAC, Cordoba, Argentina</affiliation>
    </creator>
  </creators>
  <titles>
    <title>HH137 and 138: discovering new knots and a molecular outflow with Gemini and APEX</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2017</publicationYear>
  <dates>
    <date dateType="Issued">2017-07-12</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Poster</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/826357</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.826356</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/starformation2017</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&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;
whole complex.&lt;/p&gt;</description>
  </descriptions>
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