3D Radiative Transfer Modelling and Virial Analysis of Starless Cores in the B10 Region of the Taurus Molecular Cloud

Samantha Scibelli, Yancy Shirley, Anika Schmiedeke +4

Low-mass stars like our Sun begin their evolution within cold (10 K) and dense ($\sim 10^5$ cm${}^{-3}$) cores of gas and dust. The physical structure of starless cores is best probe…