Detection of the thermal radio continuum emission from the G9.62+0.19-F Hot Core

Details Detection of the thermal radio continuum emission from the G9.62+0.19-F Hot Core Detection of the thermal radio continuum emission from the G9.62+0.19-F Hot Core

2000-06-15

arxiv.org/abs/astro-ph/0006211v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figs, A&A Letters, in press

Scientific paper

We 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.

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