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

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dc.creatorTesti, L.
dc.creatorHofner, P.
dc.creatorKurtz, S.
dc.creatorRupen, M.
dc.date2000-06-15
dc.date.accessioned2026-07-07T01:53:58Z
dc.date.available2026-07-07T01:53:58Z
dc.descriptionWe 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.
dc.description4 pages, 3 figs, A&A Letters, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0006211
dc.identifierhttp://arxiv.org/abs/astro-ph/0006211
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1171
dc.subjectAstrophysics
dc.titleDetection of the thermal radio continuum emission from the G9.62+0.19-F Hot Core
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