SMA observations of the W3(OH) complex: Dynamical differentiation between W3(H2O) and W3(OH)

We present Submillimeter Array observations of the HCN (3–2) and HCO+ (3–2) molecular lines towards the W3(H2O) and W3(OH) star-forming complexes. Infall and outflow motions in the W3(H2O) have been characterized by observing HCN and HCO+ transitions. High-velocity blue/red-shifted emission, tracing...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2016-03, Vol.456 (3), p.2681-2691
Main Authors: Qin, Sheng-Li, Schilke, Peter, Wu, Jingwen, Liu, Tie, Wu, Yuefang, Sánchez-Monge, Álvaro, Liu, Ying
Format: Article
Language:English
Subjects:
Accretion disks
Kinematics
Star & galaxy formation
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