Press Release

New Technique Narrows Hunt for Gamma-Ray Blazars

By SpaceRef Editor
May 30, 2003
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NASHVILLE — In the quest to peel back the mysteries of some of the most
compelling physics in the cosmos, the enigmatic high-energy gamma-ray blazar —
a jet spouting from a giant black hole — promises new insight into some
astrophysical phenomena that, tantalizingly, seem to be just beyond the grasp of
astronomers.

But pinpointing such blazars with ground-based gamma-ray telescopes, the kind of
telescope that might reveal some of the tightly held secrets of the rare, very
high-energy gamma-ray species of blazar, is a difficult, highly inefficient
process. Few are known.

Now, however, thanks to new optical techniques developed by a team of
astronomers at the University of Wisconsin-Madison, the world’s gamma-ray
telescopes may be able to quickly zoom in on this unusual type of blazar instead
of wasting valuable telescope time searching the skies for their telltale
signatures.

In general, blazars are a class of information-rich objects that can shine
across the electromagnetic spectrum — from radio to very high-energy gamma rays
in some cases. In the optical, most look very much like a star, a simple point
of light in the sky. Most blazars are found at cosmological distances, billions
of light years away.

A species that may be especially rich in information is known as the TeV
gamma-ray blazar because it emits gamma rays at extremely high energies. Some of
these high-end blazars are relatively close at hand, a mere 300 million light
years from Earth. But when gamma-ray telescopes scan the sky, they have a hard
time homing in on the point sources that may be emitting the gamma rays.

"With gamma-ray telescopes, you can observe a source for three months before you
get a signal," says Ramotholo Sefako, a UW-Madison astronomer who, with
Wisconsin colleague Eric Wilcots, today (May 28) presented research results that
could make it far easier for astronomers to find TeV blazars. With these new
techniques, "we can tell which objects are likely to be high-energy objects. Our
aim is to correlate optical and gamma-ray results," Sefako says.

The astronomers, who used the 1.0-meter telescope at the South African
Astronomical Observatory, shared their findings at the 202nd meeting of the
American Astronomical Society in Nashville. The team presented results on
observations of eight objects and described optical techniques that would cut
the identification time for a high-energy blazar from three months to a day.

The ability to quickly home in on blazars emitting gamma rays at TeV energies
using ground-based optical telescopes promises a wealth of new objects for study
by astronomers using gamma-ray telescopes. With more known high-energy gamma ray
blazars to choose from, astronomers can use scarce gamma-ray telescope time to
study what are considered to be some of the most unusual objects in the cosmos
instead of spending time combing the skies for them.

Blazars exist at the cores of galaxies. And while no one knows for sure what
lies at their cores, current thinking is that an enormous black hole — perhaps
a billion times more massive than the sun — creates light-years-long jets of
plasma that stick out from the poles of a torus created by an accreting disk of
material spinning into the black hole. It is these jets that are believed to be
the source of the high-energy gamma rays that interest astronomers.

Viewed at the right angle, blazars could provide a unique window to a black
hole, says Wilcots: "The jet may be a way to get a look right down to the core,
a view that is otherwise obscured by the torus of these objects."

An ability to drill down to the core of these objects, Sefako notes, may yield
insight into the physics of black holes, including a more detailed understanding
of accretion disks behavior, the physics of the jets themselves and perhaps even
be the key to discovering the origin of cosmic rays.

SpaceRef staff editor.