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

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

2003-08-21

arxiv.org/abs/astro-ph/0308387v1

Astronomy and Astrophysics

Astrophysics

8 pages, 4 figures, Proceedings to the IAU221 Star Formation at high angular resolution

Scientific paper

(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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