The University of MichiganNews Services
The University Record Online
search
Updated 10:00 AM July 10, 2006
 

front

accolades

briefs

view events

submit events

UM employment


obituaries
police beat
regents round-up
research reporter
letters


archives

Advertise with Record

contact us
meet the staff
contact us
contact us

  Research
Scientists find the reason for black holes' light shows
This artist's representation shows how magnetic fields may drive a wind in the black hole designated GRO J1655-40. Rotation and magnetic actions in the disk can cause magnetic fields to become coiled up like a snake, shown here as black lines. This can result in gas being driven upward and away from the disk by pressure created by the magnetic fields, resulting in the wind observed by Chandra. (Photo courtesy NASA/CXC/M.Weiss)
An X-ray spectrum obtained by Chandra observations. The dips seen in the spectrum are produced by absorption from a wide variety of atoms in the gas around the black hole, ranging from oxygen to nickel. A detailed study of these absorption features shows that the atoms are highly ionized and are moving away from the black hole in a high-speed wind. The conclusion of this study is that this wind is driven by magnetic fields.(Photo courtesy NASA/CXC/U.Michigan/J.Miller et al)

A U-M-led team of astronomers may know how black holes are lighting up the Universe. New data from NASA's Chandra X-ray Observatory show, for the first time, that powerful magnetic fields are the key to these brilliant and startling light shows.

It is estimated that up to half of the total radiation in the universe since the Big Bang comes from material falling toward super-massive black holes. For decades, scientists have struggled to understand how black holes, the darkest objects in the Universe, can generate such prodigious amounts of radiation.

New X-ray data from Chandra give the first clear explanation for what drives this process: magnetic fields. Chandra observed a black hole system in our galaxy, known as GRO J1655-40 (J1655, for short), where a black hole was pulling material from a companion star into a disk. "By intergalactic standards, J1655 is in our backyard so we can use it as a scale model to understand how all black holes work, including the monsters found in quasars," says Jon Miller, assistant professor of astronomy, whose paper on these results appears in this week's issue of the journal Nature.

If gas in a disk around a black hole loses energy, it will swirl toward the hole, generating light along the way. Scientists long have thought that magnetic fields may drive this energy loss by generating friction in the gas and driving a wind from the disk that carries momentum outward, in an example of conservation of momentum.

By using Chandra spectra, that is, the amount of X-rays at different energies, Miller and his team showed that the speed and density of the wind from the disk in J1655 corresponded to computer simulation predictions for winds driven by magnetic fields. The spectral fingerprint also ruled out the two other major competing theories to magnetically-driven winds.

"In 1973, theorists came up with the idea that magnetic fields could drive the generation of light by black holes," says co-author John Raymond of the Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, Mass. "Now, over 30 years later, we finally may have proof." This deeper understanding of how black holes accrete matter also teaches astronomers about other properties of black holes, including how they grow.

"Just as a doctor wants to understand the causes of an illness and not merely the symptoms, astronomers try to understand what causes phenomena they see in the universe," says co-author Danny Steeghs, also of the CfA. "By understanding what makes material fall onto black holes and its energy released, we also may learn how it plunges onto other important objects."

In addition to accretion disks around black holes, magnetic fields may play an important role in disks detected around young Sun-like stars where planets are forming, as well as ultra-dense objects called neutron stars.

NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra program for the agency's Science Mission Directorate. The Smithsonian Astrophysical Observatory controls science and flight operations from the Chandra X-ray Center, Cambridge, Mass. For information on Miller, visit www.astro.lsa.umich.edu/~jonmm/.

More Stories