Mysterious Milky Way filaments point to central black hole

Milky Way filaments: Patch of hundreds of mostly radial, thin, colorful streaks, of different lengths (fewer long ones).
View larger. | A new view toward the heart of our Milky Way galaxy, via the MeerKAT radio telescope in South Africa. The color-coding shows the position angles of the mysterious Milky Way filaments, which can be seen to spread out like spokes on a wheel from our galaxy’s central supermassive black hole, Sagittarius A*. Image via MeerKAT/ Northwestern University.

Northwestern University published this story on June 2, 2023. Edits by EarthSky.

Mysterious Milky Way filaments

We can’t see into the center of our Milky Way galaxy in visible light. Located some 25,000 light-years from Earth, it’s hidden from view by great clouds of gas and dust. But probes of the galaxy at other wavelengths have revealed a central supermassive black hole, called Sagittarius A* or Sag A* (pronounced Sag A-star). The black hole has some 4 million times our sun’s mass.

And, in the early 1980s, astronomer Farhad Yusef-Zadeh of Northwestern University in Illinois used radio telescopes to discover gigantic, one-dimensional filaments dangling vertically near Sag A*. And on Friday (June 2, 2023), Northwestern announced that Yusef-Zadeh now has seen something else. He has spied hundreds of filaments along the galactic plane – like threads, visible at radio wavelengths – measuring some 5 to 10 light-years in length. These threads spread out like spokes on a wheel from the black hole. Yusef-Zadeh commented:

I was actually stunned when I saw these.

The new population of filaments or threads are much shorter than those first discovered by Yusef-Zadeh in the 1980s. Yusef-Zadeh and his collaborators believe the structures likely originated a few million years ago as outflow from our supermassive black hole interacted with surrounding materials. Their statement explained:

Although the two populations of filaments share several similarities, Yusef-Zadeh assumes they have different origins. While the vertical filaments sweep through the galaxy, towering up to 150 light-years high, the horizontal filaments look more like the dots and dashes of Morse code, punctuating only one side of Sagittarius A*.

The Astrophysical Journal Letters published the new study on June 2. The study is titled The population of the galactic center filaments: Position angle distribution reveal a degree-scale collimated outflow from Sgr A* along the galactic plane.

It was a surprise

Yusef-Zadeh explained in a statement:

It was a surprise to suddenly find a new population of structures that seem to be pointing in the direction of the black hole. I was actually stunned when I saw these. We had to do a lot of work to establish that we weren’t fooling ourselves.

And we found that these filaments are not random but appear to be tied to the outflow of our black hole. By studying them, we could learn more about the black hole’s spin and accretion disk orientation.

It is satisfying when one finds order in a middle of a chaotic field of the nucleus of our galaxy.

Decades in the making

This study builds on four decades of Yusef-Zadeh’s research. After first discovering the vertical filaments in 1984 with Mark Morris and Don Chance, Yusef-Zadeh along with Ian Heywood and their collaborators later uncovered two gigantic radio-emitting bubbles near Sagittarius A*. Then, in a series of publications in 2022, Yusef-Zadeh (in collaboration with Heywood, Richard Arent and Mark Wardle) revealed nearly 1,000 vertical filaments, which appeared in pairs and clusters, often stacked equally spaced or side by side like strings on a harp.

Yusef-Zadeh credits the flood of new discoveries to enhanced radio astronomy technology, particularly the South African Radio Astronomy Observatory’s (SARAO) MeerKAT telescope. To pinpoint the filaments, Yusef-Zadeh’s team used a technique to remove the background and smooth the noise from MeerKAT images in order to isolate the filaments from surrounding structures. He commented:

The new MeerKAT observations have been a game changer. The advancement of technology and dedicated observing time have given us new information. It’s really a technical achievement from radio astronomers.

Horizontal vs vertical filaments

After studying the vertical filaments for decades, Yusef-Zadeh was shocked to uncover their horizontal counterparts, which he estimates are about 6 million years old. He said:

We have always been thinking about vertical filaments and their origin. I’m used to them being vertical. I never considered there might be others along the plane.

While both the vertical and horizontal populations comprise one-dimensional filaments that can be viewed with radio waves and appear to be tied to activities in the galactic center, the similarities end there.

The vertical filaments are perpendicular to the galactic plane. The horizontal filaments are parallel to the plane but point radially toward the center of the galaxy where the black hole lies. The vertical filaments are magnetic and relativistic. The horizontal filaments appear to emit thermal radiation. The vertical filaments encompass particles moving at speeds near the speed of light. The horizontal filaments appear to accelerate thermal material in a molecular cloud.

There are several hundred vertical filaments and just a few hundred horizontal filaments.

And the vertical filaments, which measure up to 150 light-years high, far surpass the size of the horizontal filaments, which measure just 5 to 10 light-years in length. The vertical filaments also adorn space around the nucleus of the galaxy; the horizontal filaments appear to spread out to only one side, pointing toward the black hole. Yusef-Zadeh said:

One of the most important implications of radial outflow that we have detected is the orientation of the accretion disk and the jet-driven outflow from Sagittarius A* along the galactic plane.

‘Our work is never complete’

The new discovery is filled with unknowns, and Yusef-Zadeh’s work to unravel its mysteries has just begun. For now, he can only consider a plausible explanation about the new population’s mechanisms and origins. He said:

We think they must have originated with some kind of outflow from an activity that happened a few million years ago. It seems to be the result of an interaction of that outflowing material with objects near it. Our work is never complete. We always need to make new observations and continually challenge our ideas and tighten up our analysis.

Bottom line: Mysterious Milky Way filaments – found by the MeerKAT telescope in South Africa – appear to point to the supermassive black hole at our galaxy’s heart.

Source: The population of the galactic center filaments: Position angle distribution reveal a degree-scale collimated outflow from Sgr A* along the galactic plane

Via Northwestern University

June 6, 2023

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