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.

MARC21 XML Export

<?xml version='1.0' encoding='UTF-8'?>
<record xmlns="">
  <controlfield tag="005">20200120144703.0</controlfield>
  <controlfield tag="001">826357</controlfield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="u">CONICET, Argentina</subfield>
    <subfield code="a">Cappa, C.E.</subfield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="u">OAC, Cordoba, Argentina</subfield>
    <subfield code="a">Gomez, M.</subfield>
  <datafield tag="856" ind1="4" ind2=" ">
    <subfield code="s">5071077</subfield>
    <subfield code="z">md5:42c43550b0132007c31a01a3375ccf15</subfield>
    <subfield code="u"></subfield>
  <datafield tag="542" ind1=" " ind2=" ">
    <subfield code="l">open</subfield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2017-07-12</subfield>
  <datafield tag="909" ind1="C" ind2="O">
    <subfield code="p">openaire</subfield>
    <subfield code="p">user-starformation2017</subfield>
    <subfield code="o"></subfield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="u">OAC, Cordoba, Argentina</subfield>
    <subfield code="a">Ferrero, L.V.</subfield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">HH137 and 138: discovering new knots and a molecular outflow with Gemini and APEX</subfield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">user-starformation2017</subfield>
  <datafield tag="540" ind1=" " ind2=" ">
    <subfield code="u"></subfield>
    <subfield code="a">Creative Commons Attribution 4.0 International</subfield>
  <datafield tag="650" ind1="1" ind2="7">
    <subfield code="a">cc-by</subfield>
    <subfield code="2"></subfield>
  <datafield tag="520" ind1=" " ind2=" ">
    <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;
whole complex.&lt;/p&gt;</subfield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="n">doi</subfield>
    <subfield code="i">isVersionOf</subfield>
    <subfield code="a">10.5281/zenodo.826356</subfield>
  <datafield tag="024" ind1=" " ind2=" ">
    <subfield code="a">10.5281/zenodo.826357</subfield>
    <subfield code="2">doi</subfield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">poster</subfield>
All versions This version
Views 4443
Downloads 3432
Data volume 172.4 MB162.3 MB
Unique views 4342
Unique downloads 3432


Cite as