Black hole accretion disk observed to 'breathe'

June 21, 2016, College of Charleston
This artist's concept depicts a supermassive black hole at the center of a galaxy. The blue color here represents radiation pouring out from material very close to the black hole. The grayish structure surrounding the black hole, called a torus, is made up of gas and dust. Credit: NASA/JPL-Caltech

Scientists may have found a link between the pulsations of light coming from a black hole accretion disk and the "breathing" of that disk.

X-ray light coming from surrounding often exhibit rhythmic pulses, referred to as quasi-periodic oscillations or QPOs, usually occurring at multiple frequencies. The exact nature of these pulses has been a mystery for over 20 years. Scientists from the College of Charleston, Observatory of Paris, and University of California, Santa Barbara, now may have an explanation for three such QPOs, observed from the X-ray binary, GRO J1655-40.

According to the model, the QPOs are attributed to natural oscillation modes of a hot, inner ring of gas near the black hole. The highest frequency QPO is attributed to the "breathing" motion of this ring. The ring expands and contracts in much the same way that human lungs do whenever a person inhales and exhales. The next highest frequency is associated with "vertical" oscillations of the ring, like a cork bobbing up and down in waves. The lowest frequency comes from the precession of the ring, as its own traces out a conical shape in space around the rotation axis of the black hole. This is the same motion that the head of a spinning top or gyroscope traces out.

All gas flows, including disks, have "natural" oscillation modes. These natural modes are generally more easily excited and have larger amplitudes than random fluctuations. "The key is to understand which natural modes are at play in any given system," says lead scientist, Prof. Chris Fragile, of the College of Charleston. In the case of GRO J1655-40, a binary system with a subgiant star in orbit around a 5 or 6 solar , the simultaneous observation of three QPOs was critical. By assuming that all three signals were coming from the same part of the accretion disk, the theorists were able to constrain the properties of that part of the disk and isolate which modes could correspond to which oscillation frequencies.

This model may help astronomers better understand black hole accretion and, ultimately, estimate the spin of black holes, an important parameter for interpreting effects related to Einstein's theory of general relativity. "Besides finding a long-sought explanation for the QPO phenomena, this discovery may provide us important details about the exact geometry of black hole accretion flows, which would be helpful in interpreting other observations," says Fragile.

This work has been accepted for publication in the Monthly Notices of the Royal Astronomical Society.

Explore further: Powerful jets from non-spinning black holes

Related Stories

Powerful jets from non-spinning black holes

November 18, 2015

A black hole is so simple (at least in traditional theories) that it can be completely described by just three parameters: its mass, its spin, and its electric charge. Even though it may have formed out of a complex mix of ...

Clocking the rotation rate of a supermassive black hole

March 10, 2016

A recent observational campaign involving more than two dozen optical telescopes and NASA's space based SWIFT X-ray telescope allowed a team of astronomers to measure very accurately the rotational rate of one of the most ...

Cosmic jets light up black hole's snack

December 16, 2015

A black hole is often thought of as a giant galactic vacuum cleaner constantly sucking in cosmic material, tearing it apart and swallowing it. So black holes should do exactly the same thing with stars, right?

Researchers find 'structure' in black hole accretion disk

March 1, 2013

(Phys.org)—A team of researchers working at the Astrophysical Institute of the Canary Islands has found evidence of a previously unknown structure in the accretion disk of a black hole that is part of an X-ray binary system. ...

Recommended for you

Making stars when the universe was half its age

January 18, 2019

The universe is about 13.8 billion years old, and its stars are arguably its most momentous handiwork. Astronomers studying the intricacies of star formation across cosmic time are trying to understand whether stars and the ...

Saturn hasn't always had rings

January 17, 2019

One of the last acts of NASA's Cassini spacecraft before its death plunge into Saturn's hydrogen and helium atmosphere was to coast between the planet and its rings and let them tug it around, essentially acting as a gravity ...

0 comments

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.