Quick Look: A New Panorama of Our Galactic Center.
The new panorama of the Galactic Center builds on previous surveys from Chandra and other telescopes. This latest version expands Chandra's high-energy view farther above and below the plane of the Galaxy - that is, the disk where most of the Galaxy's stars reside - than previous imaging campaigns.
One thread is particularly intriguing because it has X-ray and radio emission intertwined. It points perpendicular to the plane of the galaxy and is about 20 light-years long but only one-hundredth that size in width.
A new study of the X-ray and radio properties of this thread by Q. Daniel Wang of the University of Massachusetts at Amherst suggests these features are bound together by thin strips of magnetic fields. This is similar to what was observed in a previously studied thread. Such strips may have formed when magnetic fields aligned in different directions, collided, and became twisted around each other in a process called magnetic reconnection. This is similar to the phenomenon that drives energetic particles away from the Sun and is responsible for the space weather that sometimes affects Earth.
A detailed study of these threads teaches us more about the Galactic space weather astronomers have witnessed throughout the region. This weather is driven by volatile phenomena such as supernova explosions, close-quartered stars blowing off hot gas, and outbursts of matter from regions near Sagittarius A*, our Galaxy's supermassive black hole.
A panorama of the Galactic Center builds on previous surveys from Chandra and other telescopes. This latest version expands Chandra's high-energy view farther above and below the plane of the galaxy - that is, the disk where most of the galaxy's stars reside - than previous imaging campaigns. (Image: X-ray: NASA/CXC/UMass/Q.D. Wang; Radio: NRF/SARAO/MeerKAT) (click on image to enlarge)
In addition to the threads, the new panorama reveals other wonders in the Galactic Center. For example, Wang's paper reports large plumes of hot gas, which extend for about 700 light-years above and below the plane of the galaxy, seen here in greater detail than ever before. (They are much smaller than the Fermi Bubbles which extend for about 25,000 light-years above and below the plane of the galaxy.) These plumes may represent galactic-scale outflows, analogous to the particles driven away from the Sun. The gas is likely heated by supernova explosions and many recent magnetic reconnections occurring near the center of the galaxy. Such reconnection events in the Galaxy are normally not sufficiently energetic to be detected in X-rays, except for the most energetic ones at the center of the Galaxy, where the interstellar magnetic field is much stronger.
Magnetic reconnection events may play a major role in heating the gas existing between stars (the interstellar medium). This process may also be responsible for accelerating particles to produce cosmic rays like those observed on Earth and driving turbulence in the interstellar medium that triggers new generations of star birth.
The image shows that the magnetic threads tend to occur at the outer boundaries of the large plumes of hot gas. This suggests that the gas in the plumes is driving magnetic fields that collide to create the threads.
Source: Harvard-Smithsonian Center for Astrophysics
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