The flaring is not visible in optical light. It's all happening in the near-infrared, the portion of the infrared spectrum closest to optical light. Astronomers have been watching Sgr. A* for 20 years, and though the black hole does have some variability in its output, this flaring event is like nothing astronomers have observed before. This peak was over twice as bright as the previous peak flux level.
These results are being reported in the Astrophysical Journal Letters in a paper titled "Unprecedented variability of Sgr A* in NIR," and is available at the prepress site arXiv.org. The lead author is Tuan Do, an astronomer at UCLA.
The team saw Sgr. A* flaring at 75 times normal for a two-hour period on May 13th. At first, astronomer Tuan Do thought that they were seeing a star called SO-2 rather than Sgr. A*. SO-2 is one of a group of stars called S-stars that orbits the black hole closely. Astronomers have been keeping an eye on it as it orbits the black hole.
In an interview with ScienceAlert, Do said, "The black hole was so bright I at first mistook it for the star S0-2, because I had never seen Sgr A* that bright. Over the next few frames, though, it was clear the source was variable and had to be the black hole. I knew almost right away there was probably something interesting going on with the black hole."Here's a timelapse of images over 2.5 hr from May from @keckobservatory of the supermassive black hole Sgr A*. The black hole is always variable, but this was the brightest we've seen in the infrared so far. It was probably even brighter before we started observing that night! pic.twitter.com/MwXioZ7twV— Tuan Do (@quantumpenguin) August 11, 2019
This is our best-yet image of an actual black hole. It’s the super-massive black hole at the center of galaxy M87, and it was captured by the Event Horizon Telescope (EHT). The black hole itself can’t actually be seen so this image is actually of its event horizon. The EHT’s next target is Sgr. A*. Credit: Event Horizon Telescope Collaboration
The question is, what made Sgr. A* flare like this? At this point, astronomers aren't certain what caused the flaring. Sgr. A* has exhibited flaring before, just not as brightly. So flaring itself isn't unprecedented.
The group of stars that orbit close to Sgr. A* are called S stars. SO-2 made it’s closest approach about a year before the flaring observed in May 2019. Credit: Cmglee – Own work, CC BY-SA 3.0
The second possibility is where things get interesting: Something has changed in the black hole's neighborhood.
The previously mentioned star SO-2 is a prime candidate. It's one of two stars that approach very closely to Sgr. A* in an elliptical orbit. Every 16 years, it's at its closest. In the middle of 2018 was its last closest approach, when it was only 17 light-hours away from the black hole.
It's possible that SO-2's close approach disrupted the way that material flows into Sgr. A*. That would generate the kind of variability and bright flaring that astronomers saw in May, about one year after the star's close approach.
continued at: https://phys.org/news/2019-08-milky-black-hole-flared-bright.html
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