The interferometric surveys are labeled with the filled symbols and the single-dish surveys by open symbols. GASKAP-HI : ref. [2]; THOR-HI : ref. [5]; CGPS: ref. [3]; VGPS: ref. [1]; SGPS: ref. [4]; GALFA-HI : ref. [10]; EBHIS: ref. [7]; GASS: ref. [8]; HI4...
Aside from these lines of evidence, astronomers are also using their tools in ingenious ways to map the structure of the Milky Way. Just this year, scientists used two radio astronomy projects from different parts of the globe to measure theparallaxes– differences in the...
In cataloging these bubbles for subsequent analysis, Milky Way Project members can help astronomers understand both the interstellar medium and the stars themselves imaged by the survey. It will also help them to make a map of the Milky Way’s stellar formation regions. As with the other Zoonive...
Figure 1. The edge-on view of the log-scaled density projection map of the stellar, dark matter and gas components in the main galaxy system within its virial radius in the “C−4” simulation at redshift 𝑧=0z=0. Figure 2. The face-on and edge-on views of the density projecti...