A Patchy Galaxy: Unraveling the Flocculent Structure of the Milky Way’s Inner Disk
Balser and Burton use modern hydrogen (H I) data from the HI4PI survey to reexamine the Milky Way’s inner structure. They find no evidence for the clear spiral arms expected in a Grand-design galaxy. Instead, the inner disk shows a disordered, patchy distribution of gas, suggesting that the Milky Way is a flocculent spiral with irregular, loosely connected features rather than majestic, continuous arms.
When Discs Dance: How Misaligned Binary Stars Create Unusual Spiral Arms
Rowther et al. use 3D simulations to show that moderately misaligned circumbinary discs can form unusual leading spiral arms at connection points between inner and outer discs. These spirals don’t rotate with the disc and vanish when the discs align or fully break. The effect is independent of detailed disc physics, and in some cases shadows can also launch trailing spirals, meaning both types can coexist.
Tracing the Twists and Turns of a Galaxy Like Ours: What Simulations Reveal About the Milky Way's Dynamic Heart
This study uses a detailed simulation to explore the Milky Way’s structure, showing that spiral arms are dynamic, short-lived features shaped by gas flows rather than fixed patterns. The inner bar drives much of this motion, influencing where arms form and dissolve. These findings explain why the Galaxy’s spiral structure is difficult to pin down and suggest a more chaotic process behind star formation.
Do Spiral Arms Spark Star Birth? A Deep Dive into the Star Formation Life Cycle
Romanelli et al. find that spiral arms do not trigger star formation but instead act as gas collectors. Molecular cloud lifetimes, feedback timescales, and star formation processes are similar in spiral arms and inter-arm regions. Surprisingly, star formation efficiency is slightly higher in inter-arm regions, suggesting local conditions drive star formation more than large-scale galactic structures.