No CrossRef data available.
Article contents
A hydrodynamical model for the fragmentation of the W49A star-forming region ∗
Published online by Cambridge University Press: 03 August 2017
Abstract
We present a 3-D hydrodynamical and radiative transfer simulation which suggests that the circular “necklace” of massive star formation in W49A may result from fragmentation via a ring instability during the collapse of a rotating cooling molecular cloud.
- Type
- Poster Sessions
- Information
- Copyright
- Copyright © Kluwer 1991