Destroyed Star Rains onto Black Hole, Winds Blow it Back

For Release: October 21, 2015



CXC

New details about what happens when a black hole tears apart a star have been gathered by a trio of orbiting X-ray telescopes, giving scientists an extraordinary opportunity to understand the extreme environment around a black hole.

When a star comes too close to a black hole, the intense gravity of the black hole results in tidal forces that can rip the star apart. In these events, called "tidal disruptions," some of the stellar debris is flung outward at high speeds, while the rest falls toward the black hole. This causes a distinct X-ray flare that can last for a few years.

NASA’s Chandra X-ray Observatory, Swift Gamma-ray Burst Explorer, and ESA/NASA's XMM-Newton collected different pieces of this astronomical puzzle in a tidal disruption event called ASASSN-14li, originally discovered in an optical search by the All-Sky Automated Survey for Supernovae (ASAS-SN) in November 2014.

The event occurred near a supermassive black hole estimated to weigh a few million times the mass of the sun. The black hole is located in the center of PGC 043234, a galaxy that lies about 290 million light years from Earth. This makes this event the closest tidal disruption discovered in a decade. "We have seen evidence for a handful of tidal disruptions over the years and have developed a lot of ideas of what goes on," said Jon Miller of the University of Michigan in Ann Arbor, who led the study that is described in a paper published in the latest issue of Nature. "This one is the best chance we have had so far to really understand what happens when a black hole shreds a star."

After the star is destroyed, the black hole's strong gravitational force pulls most of the remains of the star toward it. This infalling debris is heated to millions of degrees and generates a huge amount of X-ray light. Soon after this surge of X-rays, the amount of light decreases as the material falls beyond the black hole's event horizon, the point beyond which no light can escape.

Gas often falls toward black holes by spiraling inward in a disk. But how this process starts has remained a mystery. In ASASSN-14li, astronomers were able to witness the formation of such a disk by looking at the X-ray light at different wavelengths (known as the "X-ray spectrum") and tracking how that changed over time.

The researchers determined that the X-rays being produced come from material that is either very close to or is actually in the smallest possible stable orbit around the black hole.

"The black hole tears the star apart and starts swallowing material really quickly, but that's not the end of the story," said co-author Jelle Kaastra of the Institute for Space Research in the Netherlands. "The black hole can't keep up that pace so it expels some of the material outwards."

The X-ray data also suggest the presence of a wind moving away from the black hole. The wind is not moving fast enough to escape the black hole's gravitational grasp. An alternative explanation for the relatively low speed is that gas from the disrupted star is following an elliptical orbit around the black hole and is at the greatest distance from the black hole where it is traveling the slowest.

"These results support some of our newest ideas for the structure and evolution of tidal disruption events," said Cole Miller, a co-author from the University of Maryland in College Park. "In the future, tidal disruptions can provide us with laboratories to study the effects of extreme gravity."

Astronomers are hoping to find more events like ASASSN-14li, which they can use to continue to test theoretical models about how black holes affect their environments and anything that might wander too close.

These results appear in the October 22 issue of the journal Nature. NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations. Swift is managed by NASA's Goddard Space Flight Center in Greenbelt, Maryland.

An interactive image, a podcast, and a video about the findings are available at:For more Chandra images, multimedia and related materials, visit:

Media contacts:

Megan Watzke

Chandra X-ray Center, Cambridge, Mass.

617-496-7998

mwatzke@cfa.harvard.edu