How Our Largest Dwarf Galaxy Keeps the Others In Line – SkyandTelescope.com

Theres something strange about the dwarf galaxies around the Milky Way.

These smaller galaxies orbit our own, but many of their orbits align along what astronomers term the vast polar structure: a pancake-shaped plane that intersects our own crepe-thin galaxy. Out of the dozens of known satellites in the Milky Ways retinue, about half of them, maybe even more, belong to this structure, dotting the plane like raisins in the pancake. Whats more this pancake rotates, the blueberries whirling around the Milky Way in the same direction.

This alignment has puzzled astronomers since the first hints of it appeared in the 1970s. Cosmological simulations dont generally predict this effect. Some researchers have even wondered if the problem is with our understanding of dark matter or of gravity itself.

In a paper posted to the astronomy preprint arXiv, Nicols Garavito Camargo (University of Arizona) and colleagues suggest the focus ought to be on the biggest of all the little fish: the Large Magellanic Cloud (LMC).

The LMC is a massive dwarf, with at least a tenth the mass of the Milky Way. Its swinging around our galaxy for the first time on a trajectory that aligns with the vast polar structure, and it may have brought a half dozen smaller galaxies in with it. That cant be a coincidence, right? Astronomers have thought so, too, and several have suggested that the LMC has somehow inspired the mysterious polar structure.

In fact, earlier this year, Jenna Samuel (now at University of Texas, Austin) and colleagues made this case: Samuels led simulations to demonstrate that dwarf galaxies tend to align along cosmic pancakes and stay that way, at least for a while when theres a massive dwarf like the LMC in the mix.

The question is how: The LMC and its retinue are only a few of the Milky Ways many satellites, so it and its attendants cant account for the plane simply by falling in. Garavito Camargo and colleagues describe how the LMC could have affected the orbits of the other galaxies.

In short, the dwarf galaxy is throwing its weight around, affecting the Milky Way, its dark matter halo, and its satellites, all via the simple force of gravity. Not only does the dwarf pull on the other satellite galaxies ahead of it in its orbit, it also draws the material behind it into a wake. In addition, the researchers realized, they would need to account for their own place in the galaxy.

As it falls in, the LMC has pulled the Milky Way off-center. Our galaxy is enormous, though, and the shift in center of mass has taken time to travel outward. While the inner regions of the galaxy and its halo are already orbiting the new center of mass, the outer regions havent gotten the memo yet. So, from our perch in the inner galaxy, we see the outer regions rotate.

Were actually in a moving car, when we thought we were just sitting still, explains coauthor Gurtina Besla (University of Arizona). You see all these things move by you and you think theyre moving at some speed, but in fact were moving along with it and theyre actually moving slightly slower. In effect, when we see the satellite galaxies moving together in concert, some of that is simply the effect of our own motion something that we hadnt considered before.

Garavito Camargo, Besla, and colleagues combined all of these effects in a simulation of the LMCMilky Way encounter, confirming that the LMCs infall is capable of reshaping the orbits of numerous objects around the Milky Way.

Even taking all these effects together, though, they still might not fully explain the strange alignment of Milky Way satellites. Then again, they dont have to: After all, cosmological simulations do create planes of satellites, just not ones as organized as the one around the Milky Way.

The idea is that, after correcting for all these effects, the remaining plane may better resemble the structures predicted in cosmological simulations, Garavito Camargo says. All this together can create something thats kind-of weird and statistically more improbable than what you might find in a generic cosmological simulation.

The new work offers a fresh approach and one that is a very thorough and convincing piece of research, which naturally got me and others working on this issue very excited, says Marcel Pawlowski (Leibniz Institute for Astrophysics Potsdam), who wasnt involved in the new study. He maintains, however, that theres still work to be done to understand the structures origin.

Advertisement

Excerpt from:

How Our Largest Dwarf Galaxy Keeps the Others In Line - SkyandTelescope.com