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

H. Beuther
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Abstract

(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.

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H. Beuther. 2003-08-21. (Sub-)mm interferometry in massive star-forming regions. https://arxiv.org/abs/astro-ph/0308387

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