We carry out an ALMA N2D+(3-2) and 1.3~mm continuum survey towards 32 high mass surface density regions in seven Infrared Dark Clouds with the aim of finding massive starless cores, which may be the initial conditions for the formation of massive stars. Cores showing strong N2D+(3-2) emission are expected to be highly deuterated and indicative of early, potentially pre-stellar stages of star formation. We also present maps of these regions in ancillary line tracers, including C18O(2-1), DCN(3-2) and DCO+(3-2). Over 100 N2D+ cores are identified with our newly developed core-finding algorithm based on connected structures in position-velocity space. The most massive core has ∼70M⊙ (potentially ∼170M⊙) and so may be representative of the initial conditions for massive star formation. The existence and dynamical properties of such cores constrain massive star formation theories. We measure the line widths and thus velocity dispersion of six of the cores with strongest N2D+(3-2) line emission, finding results that are generally consistent with virial equilibrium of pressure confined cores.
@article{arxiv.1609.06008,
title = {A Hunt for Massive Starless Cores},
author = {Shuo Kong and Jonathan C. Tan and Paola Caselli and Francesco Fontani and Mengyao Liu and Michael J. Butler},
journal= {arXiv preprint arXiv:1609.06008},
year = {2017}
}