CO clouds in the Galactic Center from NANTEN Virtual Observatory Resource

Authors
  1. Takeuchi T.
  2. Yamamoto H.
  3. Torii K.
  4. Kudo N.
  5. Hayakawa T.
  6. Kawamura A.,Mizuno N.
  7. Onishi T.
  8. Mizuno A.
  9. Ogawa H.
  10. Fukui Y.
  11. Published by
    CDS
Abstract

In order to better understand molecular clouds and their properties toward the Galactic center region, we have analyzed the NANTEN database of ^12^CO (J=1-0) and ^13^CO (J=1-0) to search for associations with candidates for young high-mass star-forming regions, such as IRAS point sources, radio continuum sources, recombination line sources, maser line sources, and other molecular line sources. We have also compared the data with TeV gamma-ray sources. The analyzed region covers -12{deg}<=l<=12{deg} and -1.5{deg}<=b<=1.5{deg} for ^12^CO, and -6{deg}<=l<=8{deg} and -1{deg}<=b<=1{deg} for ^13^CO. As a result, we identified 167 IRAS point sources, 73 recombination line sources, 58 maser sources, 107 radio continuum sources, and 77 molecular line sources associated with 169 positions with the CO emission.

Keywords
  1. molecular-clouds
  2. radio-astronomy
  3. co-line-emission
Bibliographic source Bibcode
2010PASJ...62..557T
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASJ/62/557
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PASJ/62/557

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http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASJ/62/557
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http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASJ/62/557
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https://vizier.iucaa.in/viz-bin/conesearch/J/PASJ/62/557/table1?
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IVOA Cone Search SCS
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http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASJ/62/557/table2?

History

2010-10-06T07:50:54Z
Resource record created
2010-10-06T07:50:54Z
Created
2017-10-13T15:41:20Z
Updated

Contact

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CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr