Imagine the Universe!
Imagine Home | Science |

Gamma-rays from Black Holes and Neutron Stars

Unlike gamma-ray emitting radio pulsars which shine on their own, there are a large number of galactic neutron stars and black holes which owe their gamma-ray light to the effect of a companion star. Matter from the normal star in a binary system can be caught by the gravitational field of the compact star. When this matter falls onto the neutron star or black hole, a large amount of energy is released. In fact, this process of accretion is more efficient at releasing energy than even nuclear processes.

Accretion of matter from a companion star onto a compact object

These are low-energy gamma-ray sources, emitting radiation up to a few hundred keV. Generally, this emission is the high-energy "tail" of the spectrum which is detected by X-ray experiments. Some of these sources are the so-called "X-ray pulsars". The accreted matter is funneled down onto the magnetized poles of the neutron star and we see this beam of emission as the neutron star rotates - much like a lighthouse. Black hole sources or neutron stars whose magnetic fields are much weaker (preventing them from focusing the matter onto the magnetic poles) do not emit such pulsations. All of these sources, however, are highly variable because the fuel available for accretion can change dramatically. The flux can change many orders of magnitude, and go from being undetectable to one of the brightest sources on the sky.

Outburst of GRO J0422+32
GRO J0422+32 in quiescence
GRO J0422+32 in outburst
GRO J0422+32 in quiescence
These two images show the variability which is characteristic of galactic binary systems. The left-hand picture shows the Crab pulsar, which is a source of constant flux, dwarfed by the bright outburst of a binary system dubbed GRO J0422+32. As the outburst fades, the right-hand picture shows the Crab again dominating the sky. Observations at optical, X-ray, and gamma-ray wavelengths indicate that GRO J0422+32 may include a black hole.

These binaries can turn off for decades, and new ones are always being found. Gamma-ray observations help astronomers understand the basic physics of these sources by measuring the energy and variability of the highest energy radiation coming from these sources, radiation which often comes directly from the central engine. Monitoring the sky for these objects helps scientists to gain insight into how binary systems evolve.

If words seem to be missing from the articles, please read this.

Imagine the Universe! is a service of the High Energy Astrophysics Science Archive Research Center (HEASARC), Dr. Alan Smale (Director), within the Astrophysics Science Division (ASD) at NASA's Goddard Space Flight Center.

The Imagine Team
Project Leader: Dr. Barbara Mattson
Curator: Meredith Gibb
Responsible NASA Official: Phil Newman
All material on this site has been created and updated between 1997-2014.
This page last updated: Monday, 27-Sep-2004 11:26:11 EDT