Calculated properties of the 179 resolved ATLASGAL star-forming clumps with distance measure.

The calculated properties of the 179 resolved ATLASGAL star-forming clumps with distance measure were used to study the influential roles of gravity, turbulence, and magnetic fields in shaping the physical evolution of dense massive clumps. Column 1 is the ATLASGAL name, column 2 is the clump mass, column 3 is the surface density, column 4 is the one-dimensional velocity dispersion, and column 5 is the virial parameter. Columns 6 and 7 are the semi-major and the semi-minor axes, respectively. Column 8 is the linear size, column 9 is the turbulent pressure, column 10 is the gravitational pressure, column 11 is the turbulent kinetic energy transfer rate per unit volume, and columns 12 and 13 refer to the molecular line tracer and clumps evolutionary phase, respectively.