(Sub-)mm interferometry in massive star-forming regions
天体物理学
2007-05-23 v1
摘要
(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.
引用
@article{arxiv.astro-ph/0308387,
title = {(Sub-)mm interferometry in massive star-forming regions},
author = {H. Beuther},
journal= {arXiv preprint arXiv:astro-ph/0308387},
year = {2007}
}
备注
8 pages, 4 figures, Proceedings to the IAU221 Star Formation at high angular resolution