Circumgalactic Black hole imaged by the Hubble Space Telescope

In summary, NASA has observed a possible runaway black hole that is creating a trail of stars behind it. This phenomenon is thought to be caused by the cooling of gas and subsequent star formation. The object is almost half as bright as its host galaxy and is twice the size of the Milky Way, raising questions about how the diameter of such a formation is defined.
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pinball1970
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TL;DR Summary
A "wandering" black hole thought to be the result of two merging galaxies.
From NASA:

https://www.nasa.gov/feature/goddar...-runaway-black-hole-creating-a-trail-of-stars

"We think we're seeing a wake behind the black hole where the gas cools and is able to form stars. So, we're looking at star formation trailing the black hole," said Pieter van Dokkum of Yale University in New Haven, Connecticut. "What we're seeing is the aftermath. Like the wake behind a ship we're seeing the wake behind the black hole." The trail must have lots of new stars, given that it is almost half as bright as the host galaxy it is linked to."

The milky way is 100,000 light years across, this object it twice that distance.

A Black hole facilitating the formation of new stars. The paper here :
https://iopscience.iop.org/article/10.3847/2041-8213/acba86
 
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Interesting. As a casual amateur, it's my understanding that a black hole in a galaxy is really a small part, by any measure, of a galaxy. Is that true in general and in this case?
pinball1970 said:
"What we're seeing is the aftermath. Like the wake behind a ship we're seeing the wake behind the black hole." The trail must have lots of new stars, given that it is almost half as bright as the host galaxy it is linked to."

The milky way is 100,000 light years across, this object it twice that distance.
I guess that is talking about the size of the entire thing, including the trailing stars. I wonder how the diameter is defined in such a long, drawn-out formation.
 
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FAQ: Circumgalactic Black hole imaged by the Hubble Space Telescope

What is a circumgalactic black hole?

A circumgalactic black hole is a black hole that exists in the region surrounding a galaxy, often within the galaxy's halo. These black holes can influence the dynamics and evolution of the galaxy and its surrounding matter.

How did the Hubble Space Telescope image a circumgalactic black hole?

The Hubble Space Telescope can image a circumgalactic black hole indirectly by observing the effects of the black hole on nearby matter. This includes the gravitational lensing of light from background objects and the emission of X-rays and other radiation from matter as it is accreted by the black hole.

What significance does imaging a circumgalactic black hole have for astronomy?

Imaging a circumgalactic black hole helps astronomers understand the role of black holes in galaxy formation and evolution. It provides insights into the distribution of dark matter, the behavior of high-energy phenomena, and the interactions between galaxies and their halos.

Can the Hubble Space Telescope directly observe the event horizon of a black hole?

No, the Hubble Space Telescope cannot directly observe the event horizon of a black hole. The event horizon is the boundary beyond which no light can escape, making it invisible. However, Hubble can observe the effects of the black hole on its surroundings, such as the motion of stars and gas.

What are the challenges in imaging circumgalactic black holes?

Imaging circumgalactic black holes is challenging due to their immense distances from Earth and the faintness of their signals. Additionally, distinguishing the black hole's effects from other astrophysical phenomena requires precise measurements and advanced data analysis techniques.

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