THE H II/MOLECULAR CLOUD COMPLEX W3 REVISITED: IMAGING THE RADIO CONTINUUMSOURCES USING MULTI-CONFIGURATION, MULTI-FREQUENCY OBSERVATIONS WITH THE VL A

@inproceedings{Tieftrunk1997THEHI,
  title={THE H II/MOLECULAR CLOUD COMPLEX W3 REVISITED: IMAGING THE RADIO CONTINUUMSOURCES USING MULTI-CONFIGURATION, MULTI-FREQUENCY OBSERVATIONS WITH THE VL A},
  author={Achim R. Tieftrunk and Ralph A. Gaume and Mark J. Claussen and Thomas Lambert Wilson and Kenneth J. Johnston},
  year={1997}
}
The H ii/molecular cloud complex W3 has been imaged at 4.9 GHz, 14.9 GHz and 22.5 GHz in the radio continuum and the H66α radio recombination line with subarcsecond angular resolution using combined multiple VLA configurations. Several hypercompact continuum sources with diameters ≤ 1000 AU have been detected toward IRS 4 and IRS 5, reminiscent of the “Orion Radio Zoo”. They have been imaged with a maximum angular resolution of 0. ′′1. From the flux densities at 1.3 cm, 2 cm and 6 cm we… CONTINUE READING

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The H ii/molecular cloud complex W3 revisited

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