Comparison of Prestellar Core Elongations and Large-scale Molecular Cloud Structures in the Lupus I Region
Turbulence and magnetic fields are expected to be important for regulating molecular cloud formation and evolution. However, their effects on sub-parsec to 100 parsec scales, leading to the formation of starless cores, are not well understood. We investigate the prestellar core structure morphologies obtained from analysis of the Herschel-SPIRE 350
Poidevin, F. et al.
Advertised on:
8
2014