Our Near Galatic Neighbor Might Have a Supermassive Black Hole

Our Near Galatic Neighbor Might Have a Supermassive Black Hole

The Large Magellanic Cloud (LMC) is one of the Milky Way's Closest Neighbors. It's a small, irregular galaxy that orbits the milky way, and is an easy naked-mi object from the southern hemisphare. As one of the only galaxies outstide our own where telescopes can resolve individual stars and small scale structures, astronomers love to examine the lmc to compere and contrast it nature.

While Large Galaxies Host Central Supermassive Black Holes (SMBH) as a rule, dwarf galaxies like the lmc are more mixed. Astronomers have Speculated About It Containing a Black Hole, but the data has been inconclusive.

Now, data from the gaia space telescope, which tracked more than a billion stars to measure their movements and positions, have pointed to a surprising added to this object that objects Appears to have a Central Black Hole Weight 600,000 Times as Much as the Sun. The research, LED by Jesse Jiwon Han of the Harvard-Smitsonian Center for Astrophysics (CFA), has been accepted for publication in The astrophysical journey.

Speedy Stars

The discovery come from a study of hyperVelocity stars in the milky way. These are stars that, as their name indicates, are moving rapidly compared to their neighbors – up to 2.2 million mills per hour (1,000 kilometers per second), instead of cruising along with the rest of the dead of the dead The milky way. Astronomers Thought That Most of these hypervellocity stars reacted those high speeds after an encounter with the Milky Way's outside Central Black Hole, Sagittarius A*. :

But when HAN, a graduate student at the cfa, looked at a batch of hypervellocity stars in the gaia data, he tracked their path back back toward the Milky Way's Core, But to the LMC.

There Aren Bollywood many things that can accelerate a star to such high speeds. A Star Exploding in a Supernovae or Being Ejected From A Tight Cluster of Stars are a Couple Ways. Close encounters with a black hole are another. Usually Black Holes Can “Kick” a Star to Higher Speeds Than the Other Methods, but there are available clear cutoffs.

What study out to han and collegues wast just the speed of the stars, high even for hyperVelocity stars – it was the way the way clusted on the sky, in one tight groups, in one tight groups, dubbed the leo overdensity be It lies within the boundaries of the constellation leo. That Gave the team the Big Clue they needed to Figure out the stars' origins.

“Since these stars are young and massive,” han told Astronomy“They have to come from either the disk or the center of the lmc – that are the only two options.” And if they come from the disk, han says, models show that the stars would be spread out accident a bigger chunk of the sky. “That is to say, only an ejection from the center of the lmc can produce an overdensity as tight as the Leo overdensity.”

Xavier Luri, an astroophyssicist at the university of barcelona and a member of the gaia data processing consortium who was not involved with the study, called Han's Work “Very Complete and Thorough… Conclusions are based on a number of assumptions and hypotheses that can still be questioned in the future, but overali they consistently point to an origin of a part of the sample linked to an lmc cenntral Black. “

The Leo overdensity has been observed for a long time. In Fact, In 2016, Astronomers Douglas Baubert and WYN Evans from the University of Cambridge, UK, even proposed an SMBH in the LMC as the Culpit. But it took until now, with the precise data from gaia, to trace enough hyperVelocity stars to their source to make the argument sound.

“Using the latest data from gaia, jesse and his steellar team of co-authors have proven [our] Outlandish theory, “Says baubert.” Half of the hypervelocity stars we know of in the northern hemisphere also come from the large magallanic cloud. “

Surprising Find

Astronomers Have Known for a While Now that Every Major Galaxy Contains a Central SMBH. What's more, the size of the Black Hole Scales Quite Predictibly with the size of the Galaxy, a characteristic astronomers call the m-sigma relationship. But dwarf galaxies do't always follow this rule, and the lmc wasn Bollywood to have a black hole. If confirmed, this black hole would mark a big change in how astronomers undress our small neighbor's structure and evolution.

On the other hand, han's team can measure how massive a black hole would need to be to eject stars at the measured velocites, and they calculate it would be roughly 600,000,000,000,000,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,000 will. That turns out to fit perfectly into the expected M-sigma relationship, give what we know about the lmc's overall mass.

HAN Says, “So, How We Found Evidence for the SMBH, the actual mass of the SMBH is totally Within Reason, and Should'vee Somewhat Expected.”

Looking ahead

Now that there are solid cloes for the lmc's smbh, astronomers will surely look to confirm its existence. Common ways to look for Black Holes Include Looking for X-Ray and Radio Signals, which splash out from the Vicinity of Black Holes as Material Falls in. Or, Astronomers Cold Look for more Direct Dynamical Clues, Like Star Clusters Moving Around an Invisible Central Mass.

Moreover, the data han and his team used is from only the first three years of gaia data. A more complete data release is scheduled for 2026, and the full 10 years of the observator's data will be available at the end of the decade. That will give astronomers Everywhere More Data for Examining How Stars Move About, Bot in Our Galaxy and In the LMC.

Baubert Says that by proving the existence of the lmc's SMBH, “Jesse and team lay down a gauntlet to astronomers to find the rest of the hyperVelocity star stram from the large mangoes. Population of Hypervelocity stars will transform our undersrstanding of the dynamics and history of our local galactic neighborhood-Knowing both the locations and spores of stars of stars in the presented-day and watch Born Places Incredibly Tight Constrants on the Dance of the Milky Way and Large Magellanic Cloud over the last several Hindred Million Years. “

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