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Great Balls of Fire: Star Formation in Gas Clouds Accelerated by a Hot Wind

  • Authors: Stephanie Tonnesen, Rory Smith, Bianca Poggianti, Benedetta Vulcani, Nina Akerman, Marco Gullieuszik, Eric Giunchi, Antonino Marasco, Alessandro Ignesti

Stephanie Tonnesen et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 11.

vz,init versus tinit for star particles whose velocity changes by more than 5 km s−1, color-coded by their velocity change. The solid black line is the mass-weighted average velocity of the full stellar population. Stars faster than the average tend to slow down, while those slower than the average tend to speed up, particularly for the fiducial and ldcloud simulations. The gravity from the accelerating dense cloud of gas is likely responsible for the blue (accelerating) star particles that are moving faster than the average stellar velocity.

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