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posted by Fnord666 on Saturday July 29 2017, @01:36AM   Printer-friendly
from the what-about-snickers? dept.

https://news.northwestern.edu/stories/2017/july/milky-way-origin-matter-galaxy/

In a first-of-its-kind analysis, Northwestern University astrophysicists have discovered that, contrary to previously standard lore, up to half of the matter in our Milky Way galaxy may come from distant galaxies. As a result, each one of us may be made in part from extragalactic matter.

Using supercomputer simulations, the research team found a major and unexpected new mode for how galaxies, including our own Milky Way, acquired their matter: intergalactic transfer. The simulations show that supernova explosions eject copious amounts of gas from galaxies, which causes atoms to be transported from one galaxy to another via powerful galactic winds. Intergalactic transfer is a newly identified phenomenon, which simulations indicate will be critical for understanding how galaxies evolve.

"Given how much of the matter out of which we formed may have come from other galaxies, we could consider ourselves space travelers or extragalactic immigrants," said Daniel Anglés-Alcázar, a postdoctoral fellow in Northwestern's astrophysics center, CIERA (Center for Interdisciplinary Exploration and Research in Astrophysics), who led the study. "It is likely that much of the Milky Way's matter was in other galaxies before it was kicked out by a powerful wind, traveled across intergalactic space and eventually found its new home in the Milky Way."

Galaxies are far apart from each other, so even though galactic winds propagate at several hundred kilometers per second, this process occurred over several billion years.

Abstract and full journal article are available on arXiv: The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations


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  • (Score: 1) by khallow on Saturday July 29 2017, @12:35PM

    by khallow (3766) Subscriber Badge on Saturday July 29 2017, @12:35PM (#546222) Journal
    It's probably just the stellar wind and supernova residue collectively emitted by millions to billions of stars (I presume this would be from galaxies and globular clusters much smaller than the Milky Way's 100 billion or so stars). So steady state would be hydrogen and helium like the solar wind of our star system plus the occasional supernova debris. For a relatively massive galaxy like ours, most of this stuff never escapes, but it wouldn't be the same in a much smaller galaxy.