Gamma-ray Bursts Challenge Theoretical Models

September 26, 1996

WEST LAFAYETTE, Ind. -- An international team of astronomers has observed extremely rapid bursts of high-energy gamma rays from a distant galaxy, an observation that is challenging how astronomers explain such phenomena.

"This is the brightest source of high-energy gamma rays we have ever observed," says James Gaidos, professor of physics at Purdue University and a member of the research team. "In addition, the bursts were extremely rapid, with the first occurring over less than a day and the second in less than half an hour."

Previous flares observed from the distant galaxy consisted of a few gamma rays per minute hitting the team's detector over several days.

Another member of the team, John Finley, assistant professor of physics at Purdue, says the current models describing such gamma-ray flares predict that variations should occur, but on the scale of days.

"No model predicts anything happening this fast," Finley says. "These flares occurred much faster than any theory can explain at this point."

The researchers report their observations -- made during eight days in May -- in the Sept. 26 issue of the journal Nature.

In the past four years, the team of astronomers working at the Smithsonian's Fred Lawrence Whipple Observatory in Arizona has observed high-energy gamma-ray bursts coming from the active galactic nucleus known as Markarian 421, a galaxy some 400 million light-years from Earth. Gamma rays are highly energetic photons, and very high-energy gamma rays carry with them energies of trillions of electron volts, a level that is hundreds of billions of times greater than visible light.

Scientists presume that the energy engine powering Markarian 421 is a super-massive black hole at the core of the galaxy, and theorize that the gamma rays may originate in very fast-moving jets of matter that erupt from the region surrounding the black hole. A black hole is formed when stars and other material in a galaxy's core are compressed to enormous densities by gravity. The resulting gravitational field is so strong that nothing, not even light, can escape.

The researchers counted 15 gamma rays per minute during the first flare from Markarian 421, 10 times as high as the rate observed from the Crab Nebula, which is a steady source of high-energy gamma rays in our own galaxy.

By using mathematical equations that relate the duration of the flare to the size of the region emitting the bursts, Gaidos says the rapidity of the second flare suggests that the region emitting the gamma rays is extremely small on an astrophysical scale, perhaps even smaller than our solar system.

Another unusual feature of Markarian 421 is that it is bright at both the low and high ends of the energy spectrum, but emits only a weak signal in certain regions of gamma rays.

"This particular object radiates only faintly in the energy region where gamma rays have an energy of a few hundred million electron volts," explains Gaidos. "This is the region where the detector on NASA's orbiting Compton Gamma Ray Observatory makes observations.

"Just why Markarian 421 radiates in this unusual manner is a question scientists are very interested in and are currently investigating."

The research reported in the Nature paper is the result of collaborative efforts of scientists from Purdue; the Harvard-Smithsonian Center for Astrophysics; Iowa State University; the University of Michigan; the University of Leeds, United Kingdom; University College in Ireland; St. Patrick's College, Ireland; and Regional Technical College, Ireland.

Other team members from Purdue are Glenn Sembroski and Charles Wilson, senior research scientists. The research is funded by the U.S. Department of Energy. Sources: James Gaidos, (765) 494-5171; e-mail, gaidos@purdd.physics.purdue.edu
John Finley, (765) 494-5048; e-mail, finley@physics.purdue.edu
Writer: Amanda Siegfried, (765) 494-4709; e-mail, amanda_siegfried@uns.purdue.edu
Purdue News Service: (765) 494-2096; e-mail, purduenews@uns.purdue.edu

NOTE TO JOURNALISTS: A color photo of the telescope used to detect gamma ray bursts is available from Purdue News Service, (765) 494-4709. Ask for the photo called Gaidos/Gamma .
-end-


Purdue University

Related Black Hole Articles from Brightsurf:

Black hole or no black hole: On the outcome of neutron star collisions
A new study lead by GSI scientists and international colleagues investigates black-hole formation in neutron star mergers.

The black hole always chirps twice: New clues deciphering the shape of black holes
A team of gravitational-wave scientists led by the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) reveal that when two black holes collide and merge, the remnant black hole 'chirps' not once, but multiple times, emitting gravitational waves--intense ripples in the fabric space and time--that inform us about its shape.

Wobbling shadow of the M87 black hole
New analysis from the Event Horizon Telescope (EHT) Collaboration reveals the behavior of the supermassive black hole in the center of the M87 galaxy across multiple years, indicating the crescent-like shadow feature appears to be wobbling.

How to have a blast like a black hole
Scientists at Osaka University have created magnetized-plasma conditions similar to those near a black hole using very intense laser pulses.

Black hole collision may have exploded with light
Astronomers have seen what appears to the first light ever detected from a black hole merger.

Black hole's heart still beating
The first confirmed heartbeat of a supermassive black hole is still going strong more than ten years after first being observed.

Black hole team discovers path to razor-sharp black hole images
A team of researchers have published new calculations that predict a striking and intricate substructure within black hole images from extreme gravitational light bending.

Planets around a black hole?
Theoreticians in two different fields defied the common knowledge that planets orbit stars like the Sun.

Black hole mergers: Cooking with gas
Gravitational wave detectors are finding black hole mergers in the universe at the rate of one per week.

Going against the flow around a supermassive black hole
At the center of a galaxy called NGC 1068, a supermassive black hole hides within a thick doughnut-shaped cloud of dust and gas.

Read More: Black Hole News and Black Hole Current Events
Brightsurf.com is a participant in the Amazon Services LLC Associates Program, an affiliate advertising program designed to provide a means for sites to earn advertising fees by advertising and linking to Amazon.com.