Tracing the remnants of Andromeda's violent history
Collisions between galaxies create tidal artifacts with all sorts of shapes. This new work from Ivanna Escala found conclusive evidence that Andromeda's Northeast, West, and Southeast shelfs and Giant Stellar Stream are the result of a collision with another galaxy. Studying these tidal features can teach us about how galaxies grow and evolve over time as they accrete new material. Credit: NASA, ESA, Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University), K. Noll (STScI), and J. Westphal (Caltech).

An analysis of the composition and motion of more than 500 stars shows that there was a collision between Andromeda and a neighboring galaxy. The findings improved our understanding of the events that shape the evolution of the universe.

In the wake of a catastrophic crash, Galaxies grow by accretion from nearby objects. Astronomers call these stellar associations tidal features. This can include arcs or streams. The forces that shaped the appearance and makeup of a galaxy can be studied.

The movement of the stars can be used to identify the remnants of crashes. This information is used to identify stars in a collision.

She collaborated with Mark Fardal of the Space Telescope Science Institute and Puragra Guhathakurta of UC Santa Cruz.

The NE shelf is a tidal shell composed of debris from the aftermath of a collision.

Tracing the remnants of Andromeda's violent history
The Andromeda Galaxy, also known as M-31. Credit: NASA /MSFC / Meteoroid Environment Office / Bill Cook

Their work shows that the NE shelf is part of a multi-shell system with the galaxy's West and Southeast shelves and that the material in these regions is consistent with that of the giant stellar stream.

The results are in line with the model that predicted the first loop of material from a collision and the NE shelf.

This level of analysis confirms predictions about the violent past of Andromeda and informs astronomer's understanding of how material from the collision of stars shapes a galaxy's surrounding features.