Curiouser and Curiouser
March 23, 2000 -- The exotic world of gamma-ray astronomy
has taken yet another surprising turn with the revelation that
half the previously unidentified high-energy gamma ray sources
in our own galaxy, the Milky Way, actually comprise a new class
of mysterious objects.
"These are objects we've never seen before," said Dr. Neil Gehrels, an astrophysicist at NASA's Goddard Space Flight Center, Greenbelt, MD. "We can't make out what they are yet, but we know they're strange and, boy, there's a lot of them. These are very different than the famous gamma-ray burst sources, because the gamma rays shine continuously instead of coming in a flash, like the gamma-ray bursts."
Right: This simulated image shows how the sky would look to eyes sensitive to gamma radiation. [more information from Goddard Space Flight Center]
The discovery of this new class and speculation regarding
its qualities appear in the March 22 issue of Nature in an article
by Drs. Neil Gehrels, Daryl Macomb, David Bertsch, David Thompson
and Robert Hartman, all from Goddard.
The known gamma-ray universe contains 170 yet-unidentified gamma-ray sources, as listed in a 271-source catalog compiled by the Energetic Gamma Ray Telescope Experiment (EGRET) aboard NASA's Compton Gamma Ray Observatory (CGRO) spacecraft. Scientists have struggled for 20 years to associate the unidentified sources with known objects emitting other types of light. The new class reported today represents one of the first breakthroughs in their understanding.
Gehrels said that of the 170 unidentified sources in our galaxy, about half lie in a narrow band along the Milky Way plane. These may
What objects could be emitting gamma rays in the Gould Belt? Possibilities are black holes acting as particle accelerators, the massive stars themselves, and clusters of oddball pulsars, among other theories.
A black hole with jets of particles shooting away from it and toward us might be visible as gamma rays. Scientists have observed this phenomenon with EGRET in supermassive black holes, which lurk in the centers of distant galaxies, but never in smaller black holes within our own galaxy.
Left: This images comes from an animation illustrating how neutron stars in our galaxy could be a source of mysterious gamma-ray glows near the galactic plane. To view the 2.2 MB QuickTime movie, click here.
For the massive-star scenario, stars 10 to 20 times as massive as the Sun could generate stellar winds that throw high-velocity particles into the surrounding space. The particles would slam into gas atoms surrounding the star to produce gamma rays.
Rapidly spinning, magnetic neutron stars known as pulsars are yet another candidate for the mystery gamma-ray sources. An earlier finding by Drs. Jules Halpern (Columbia University, New York, NY), Stephen Holt (Goddard) and David Bertsch showed that the Geminga pulsar is detectable only in X-rays and gamma rays. Several of the EGRET unidentified gamma-ray sources could be exotic high-energy pulsars like this one. Such a discovery would radically change scientists' understanding of pulsar and neutron star populations, as the current census is based largely on those pulsars only detected by radio telescopes.
"Once again we have come face-to-face with the knowledge that the universe is unknown to us, but has patterns that lead us to understanding," said Dr. Alan Bunner, Science Director of NASA's Structure and Evolution of the Universe program. "It's an exciting feeling." Bunner said that the unidentified gamma-ray sources will remain a tantalizing mystery until the 2005 launch of GLAST, the Gamma Ray Large Area Space Telescope. Instruments aboard GLAST will be 50 times more sensitive than the EGRET instrument.Web Links
Amateurs Catch a Gamma-ray Burst -- Amateur astronomers detect afterglow from a gamma-ray burst.
High-Energy Astrophysics Workshop for
Amateur Astronomers --
meeting announcement home page
Sign-up for the AAVSO Gamma-ray Burst Network -- although this page says there is a Dec. 1, 1999 deadline, you can still register!
American Association of Variable Star Observers -- Amateur observers' home page