Physical Properties and Real Nature of Massive Clumps in the Galaxy

Physical Properties and Real Nature of Massive Clumps in the Galaxy -- SUPPLEMENTAL MATERIAL

Zu-Jia Lu, Veli-Matti Pelkonen, Mika Juvela, Paolo Padoan, Troels Haugbølle, Åke Nordlund

2022, Monthly Notices of the Royal Astronomical Society, 510, 1697

This is a large text table with one line for each of the 51,831 compact sources, and 34 columns.
See Appendix A in the paper for a detailed description of the columns.

Surface brightness maps

These are the synthetic Herschel's observations at 5 different wavelengths and 4 different distances.
With 3 snapshots and 3 directions per snapshots, we have a total of 180 maps.
The maps have been grouped into a tar file per snapshot, so each tar file has 60 maps.

Surface brightness maps for t=15.4 Myr snapshot

Surface brightness maps for t=23.3 Myr snapshot

Surface brightness maps for t=34.2 Myr snapshot

Three-color images (from the synthetic maps at 2 kpc)

(see description of the top panel of figure 2 in the paper)

t=15.4 Myr, x direction t=15.4 Myr, y direction t=15.4 Myr, z direction