Madrid. Three new studies co-led by Stanford scientists reveal that the birth of our galaxy may not be typical of how others evolved.
For decades, scientists have used the Milky Way as a model to understand how galaxies form. But a trio of new studies raise questions about whether the Milky Way is really representative of other galaxies in the universe.
The Milky Way has been an incredible laboratory, including for the physics of galaxy formation and dark matter
Risa Wechsler, professor of physics in the School of Humanities and Sciences, said in a statement. But the Milky Way is just one system and may not be typical of how other galaxies formed. That is why it is essential to find them similar and compare them.
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To achieve this, Wechsler co-founded the Satellites Around Analog Galaxies (SAGA) project, dedicated to comparing galaxies similar in mass to the Milky Way.
After more than a decade of exploring the universe, the SAGA team identified and studied 101 analog galaxies similar to the Milky Way as a first step in their ongoing research. The results, published in three studies in The Astrophysical Journalreveal that, in many ways, the evolutionary history of the Milky Way is different from that of other galaxies of comparable size.
Our results show that we cannot limit galaxy formation models to just the Milky Way.
he pointed out.
dark matter
In addition to Wechsler, the SAGA project is also led by Professor Marla Geha of Yale University and Yao-Yuan Mao, an associate professor at the University of Utah. All three are co-authors of the recently published studies.
The Milky Way is made up of ordinary atomic matter, such as hydrogen and iron. But this only represents about 15 percent of the mass of the universe. The remaining 85 is mysterious and invisible dark substance.
Nobody knows what dark matter is made of.
Wechsler said. It does not interact with ordinary or light. There’s probably dark mass circulating through you right now and you don’t even know it.
Studies show that galaxies form within massive regions of dark matter called halos.
A dark matter halo may be invisible, but its enormous size creates a gravitational force strong enough to attract ordinary matter from space and transform it into stars and galaxies.
A key goal of the SAGA survey is to determine how dark matter halos affect galactic evolution. To start, the team focused on galactic satellites, which orbit much larger host galaxies, such as the Milky Way. The researchers identified four of the brightest satellite galaxies, including the two largest, known as the Large and Small Magellanic Clouds (LMC and SMC).
They then carried out a search for satellites around other host galaxies of similar mass. Using telescopic images, they eventually identified 378 surrounding 101 Milky Way-like hosts.
There’s a reason no one has tried this before.
Wechsler said. It is a really ambitious project. We had to use clever techniques to separate those 378 orbiting galaxies from thousands of objects in the background. It’s a real needle-in-a-haystack problem.
Three studies
In one of three new SAGA studies, researchers found that the number of satellites per host galaxy ranges from zero to 13. The Milky Way’s four observable satellites fit into that range.
Large satellites
The research also revealed that host galaxies with large satellites, similar in size to the Milky Way’s massive LMC and SMC, tend to have more satellites overall.
But the Milky Way actually hosts fewer satellites than similar galaxies, making it an outlier among its peers.
A second study focused on star formation in satellite galaxies, an important metric for understanding how galaxies evolve. He found that in a typical host, the smaller satellites are still forming stars. But in the Milky Way, the formation of these only occurs in the massive LMC and SMC. All the smaller satellites have stopped forming stars.
Now we have a puzzle
Wechsler mentioned. What in the Milky Way caused these small, lower-mass satellites to see their star formation extinguished? Perhaps unlike a typical host galaxy, the Milky Way has a unique combination of older satellites that have stopped forming stars and newer, more active galaxies (the LMC and SMC) that recently fell into the dark matter halo. of the Milky Way
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The study also found that star formation generally stops in satellite galaxies located closer to the host, perhaps due to the gravitational pull of dark matter halos in and around it.
For me, the frontier is figuring out what dark matter does on scales smaller than the Milky Way, like in the smaller dark matter halos that surround these satellites.
Wechsler pointed out.
The third study, led by Stanford doctoral researcher Yunchong Wang, compares the new data with computer simulations and calls for the development of a new model of galaxy formation based in part on the SAGA survey.
The project provides a benchmark to advance our understanding of the universe through the detailed study of satellite galaxies in systems beyond the Milky Way.
Wechsler said. Although we finished our initial goal of mapping bright satellites in 101 host galaxies, there is much more work to do
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