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18 April 2024
 
  » arxiv » astro-ph/0006211

 Article overview


Detection of the thermal radio continuum emission from the G9.62+0.19-F Hot Core
L. Testi ; P. Hofner ; S. Kurtz ; M. Rupen ;
Date 15 Jun 2000
Subject astro-ph
AffiliationArcetri), P. Hofner (UPR, Arecibo), S. Kurtz (UNAM), M. Rupen (NRAO
AbstractWe present new high resolution and high sensitivity multi-frequency VLA radio continuum observations of the G9.62+0.19-F hot molecular core. We detect for the first time faint centimetric radio continuum emission at the position of the core. The centimetric continuum spectrum of the source is consistent with thermal emission from ionised gas. This is the first direct evidence that a newly born massive star is powering the G9.62+0.19-F hot core.
Source arXiv, astro-ph/0006211
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