how is the local interstellar material moving?

Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust. Soler et al. A&A submitted.

HOW is star formation distributed in the solar neighborhood?

A comparison of the Milky Way’s recent star formation revealed by dust thermal emission and high-mass stars. J.D. Soler, E. Zari, Elia D., et al. A&A 678, A95, 8

how is the interstellar GAS moving around the taurus molecular cloud?

A panoptic view of the Taurus molecular cloud. I. The cloud dynamics revealed by gas emission and 3D dust. J.D. Soler et al. A&A 675, A206, 18

 The Galactic dynamics revealed by the filamentary structure in atomic hydrogen emission

The filamentary structures in the CO emission toward the Milky Way disk

Filamentary structure in the THOR HI survey