(Sub-)mm interferometry in massive star-forming regions

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dc.creatorBeuther, H.
dc.date2003-08-21
dc.date.accessioned2026-07-07T02:09:17Z
dc.date.available2026-07-07T02:09:17Z
dc.description(Sub-)mm interferometry is the most favorable technique to investigate the earliest stages of massive star formation. I will outline general applications in that field and discuss results of different sub-topics (hot core chemistry and massive molecular outflows). Furthermore, recent data obtained with the Submillimeter Array will be shown to present the unique capabilities of this new instrument. Finally, I will give a short outlook on the main physical topics of massive star formation to be tackled with (sub-)mm interferometry within the next decade.
dc.description8 pages, 4 figures, Proceedings to the IAU221 Star Formation at high angular resolution
dc.identifierhttps://arxiv.org/abs/astro-ph/0308387
dc.identifierhttp://arxiv.org/abs/astro-ph/0308387
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6379
dc.subjectAstrophysics
dc.title(Sub-)mm interferometry in massive star-forming regions
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