Blogarchiv
Astronomie - Enormous X-ray bubbles balloon from the center of the Milky Way

11.12.2020

120820-ec-x-ray-bubble-feat-1030x580

Bubbles spill from the center of the Milky Way, seen in both gamma rays (red) and X-rays (blue). The newly found X-ray bubbles are even bigger than the previously known gamma-ray bubbles. Both sets of bubbles extend above and below the plane of the galaxy (central horizontal line).

P. PREDEHL ET AL/NATURE 2021

Two giant, mysterious bubbles spew from the Milky Way’s heart, and now it appears the bubbles may have doubles.

Scientists have known for a decade that two bubbles of charged particles, or plasma, flank the plane of the Milky Way. Those structures, known as the Fermi bubbles after the telescope that detected them, are visible in high-energy light called gamma rays (SN: 11/9/10). But now, the eROSITA X-ray telescope has revealed larger bubbles, seen in X-rays. The X-ray bubbles extend about 45,000 light-years above and below the center of the galaxy, researchers report online December 9 in Nature.

Previously, researchers had seen an X-ray arc above the galactic plane (SN: 7/8/20). But no such feature was evident below the plane of the galaxy. That lack of symmetry led some scientists to discount the possibility of X-ray bubbles. With the new results, “this argument now has fallen,” says study coauthor Andrea Merloni, an astronomer at the Max Planck Institute for Extraterrestrial Physics in Garching, Germany. The eROSITA data reveal a faint and previously unknown bubble below the galactic plane, and a matching bubble above. The gamma-ray bubbles are nested inside the X-ray bubbles, suggesting that the two features are connected, says Merloni.

Studying the bubbles could help reveal violent events that may have taken place in the galaxy’s past. The supermassive black hole at the center of the Milky Way is currently fairly quiet, as far as black holes go. But a past feeding frenzy might have spewed its leftovers outward, forming the structures. Or the bubbles could have been the result of a period when many stars formed and exploded in the galaxy’s heart. Further study of the X-ray and gamma-ray bubbles could help reveal the cause.

Quelle: Science News

1357 Views
Raumfahrt+Astronomie-Blog von CENAP 0