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  <title>W 40 Star-Forming Region Chandra X-Ray Point Source Catalog</title>
  <shortName>W40SFRCXO</shortName>
  <identifier>ivo://nasa.heasarc/w40sfrcxo</identifier>
  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Kuhn et al.</name>
    </creator>
    <contributor/>
    <date>2026-04-03</date>
    <contact>
      <name>NASA/GSFC HEASARC help desk</name>
      <email>heasarc-vo at athena.gsfc.nasa.gov</email>
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    <subject>Survey Source</subject>
    <description>
      The young stellar cluster illuminating the W40 H II region, one of the nearest massive star-forming regions (SFRs), has been observed with the ACIS detector on board the Chandra X-ray Observatory. Due to its high obscuration, this is a poorly studied stellar cluster with only a handful of bright stars visible in the optical band, including three OB stars identified as primary excitation sources. The authors detect 225 X-ray sources, of which 85% are confidently identified as young stellar members of the region. Two potential distances of the cluster, 260 pc and 600 pc, are used in the paper. Supposing the X-ray luminosity function of SFRs to be universal, it supports a 600 pc distance as a lower limit for W40 and a total population of at least 600 stars down to 0.1 M&amp;lt;sub&amp;gt;sun&amp;lt;/sub&amp;gt; under the assumption of a coeval population with a uniform obscuration. In fact, there is strong spatial variation in K&amp;lt;sub&amp;gt;s&amp;lt;/sub&amp;gt;-band-excess disk fraction and non-uniform obscuration due to a dust lane that is identified in absorption in optical, infrared, and X-ray. The dust lane is likely part of a ring of material which includes the molecular core within W40. In contrast to the likely ongoing star formation in the dust lane, the molecular core is inactive. The star cluster has a spherical morphology, an isothermal sphere density profile, and mass segregation down to 1.5 M&amp;lt;sub&amp;gt;sun&amp;lt;/sub&amp;gt;. However, other cluster properties, including a &amp;lt;= 1 Myr age estimate and ongoing star formation, indicate that the cluster is not dynamically relaxed. X-ray diffuse emission and a powerful flare from a young stellar object are also reported in the reference paper. This table was created by the HEASARC in March 2011 based on electronic versions of Tables, 1, 2 and 4 of the reference paper which were obtained from the ApJ web site. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2010ApJ...725.2485K
    </source>
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    <type>Catalog</type>
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          W 40 Star-Forming Region Chandra X-Ray Point Source Catalog
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          <name>log_lx_2_error</name>
          <description>
            Error in Log of Intrinsic Full-Band Luminosity
          </description>
          <unit>log(erg/s)</unit>
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            Error in K_S-Band Magnitude
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            stat.error;phot.mag;em.IR.K
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            Error in Log of Intrinsic Hard-Band Luminosity
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            stat.error;phys.luminosity;em.X-ray.medium
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          <flag>
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        <column>
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            2MASS Photometry Quality and Confusion Flag
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            meta.code
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          <flag>
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        <column>
          <name>exposure</name>
          <description>
            Effective Exposure (s)
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          <unit>s</unit>
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            time.duration;obs.exposure
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            nullable
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          <name>log_lx_obs</name>
          <description>
            Log of Apparent Full-Band Luminosity
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          <unit>log(erg/s)</unit>
          <ucd>
            phys.luminosity;em.X-ray
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        <column>
          <name>source_anomaly_flag</name>
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            Flag Indicates Source Anomaly
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          <ucd>
            meta.code
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            Log of Intrinsic Hard-Band Luminosity
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          <unit>log(erg/s)</unit>
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            phys.luminosity;em.X-ray.medium
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        <column>
          <name>jmag</name>
          <description>
            2MASS J-Band Magnitude
          </description>
          <unit>mag</unit>
          <ucd>
            phot.mag;em.IR.J
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          <name>off_axis</name>
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            Off-Axis Angle (arcmin)
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          <unit>arcmin</unit>
          <ucd>
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            Declination
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          <description>
            Sequential Identification Number for Each Source in Catalog
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            meta.id;src
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            Variability Characterization
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          <name>median_energy</name>
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            Median Energy of Net Counts in Full Band (keV)
          </description>
          <unit>keV</unit>
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            phys.energy
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            Error in 2MASS H-Band Magnitude
          </description>
          <unit>mag</unit>
          <ucd>
            stat.error;phot.mag;em.IR.H
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          <flag>
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        <column>
          <name>av</name>
          <description>
            Visual Absorption from J vs. J-H Diagram (mag)
          </description>
          <unit>mag</unit>
          <ucd>
            phys.absorption;em.opt.V
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        <column>
          <name>hb_counts</name>
          <description>
            Extracted Net Counts in the Hard Energy Band
          </description>
          <unit>ct</unit>
          <ucd>
            phot;em.X-ray.medium
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            System unit vector column
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        <column>
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          <description>
            Galactic Latitude
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          <unit>degree</unit>
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            pos.galactic.lat
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        <column>
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            Galactic Longitude
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          <unit>degree</unit>
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            Average 1-Sigma Uncertainty in Net Counts
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            PSF Fraction Enclosed within Extraction Region
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            Extracted Net Counts in Full Band
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            Column Density Obtained
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            Log of Intrinsic Full-Band Luminosity
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            Intrinsic Hard-Band Luminosity
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            Error in 2MASS J-Band Magnitude
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        </column>
        <column>
          <name>log_lx_2</name>
          <description>
            Intrinsic Full-Band Luminosity
          </description>
          <unit>log(erg/s)</unit>
          <ucd>
            phys.luminosity;em.X-ray
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
      </table>
    </schema>
  </tableset>
</ri:Resource>