Replication Data for: "The Per-Tau Shell: A Giant Star-Forming Spherical Shell Revealed by 3D Dust Observations" (Bialy et al. 2021)

Bialy et al. (2021) presented 2D and 3D observations of the Perseus and Taurus star-forming region, showing that the 3D ISM structure reveals the existence of a very extended shell, R~80 pc, where the Perseus and Taurus molecular clouds lie on the two ends of the shell. This shell was named "the Per-Tau Shell", and it was argued that it may have been produced by a past supernova (SN) and stellar feedback activity, pointing to the potential importance of positive SN feedback. This database includes the data required to reproduce these results, and further study this region in 2D and 3D. It includes: A) DATA: - 1 pc resolution 3D dust map (Leike et al. 2020) - Planck's E(B-V) dust (Abergel et al. 2014) - 12CO PPV cube (Dame et al. 2001) - Atomic Hydrogen (HI4PI; Bekhti et al. 2016) - H-Alpha (Finkbeiner 2003) - 26Aluminum (COMPTEL; Diehl1995) - X-ray (ROSAT; Snowden et al. 1997) - 3D masks highlighting the Perseus and Taurus molecular clouds - 3D Models of the Per-Tau Shell and the Tau Ring - 2D projections of the Per-Tau Shell model, the Tau Ring model, the HI void, the X-ray blob (identified in ROSAT and eROSITA) B) a GLUE session that may be used to conveniently reproduce the figures, and further study the region (visit https://glueviz.org/ for more info and installation). Please cite Bialy et al. (2021) ("The Per-Tau Shell: A Giant Star-Forming Spherical Shell Revealed by 3D Dust Observations") whenever using this data. Feel free to contact me for further inquiries and discussions! Shmuel