Last updated on April 18, 2014 at 21:21 EDT

Astronomers Link Old Stars and Mysterious Cosmic Explosions

December 18, 2005

Carnegie — Cosmic gamma-ray bursts, the most powerful explosions in the universe, have the extreme brilliance of a billion billion Suns and occur several times a day. But they are not all created equal. For several decades astronomers have known that two types exist–long ones that last for tens or hundreds of seconds, and short bursts, which last a few milliseconds to a second.

Intense research over the last decade has shown that long bursts are the death throes of massive stars in distant, young, and vigorously star forming galaxies. The origin of the short gamma-ray bursts, however, has been shrouded in mystery until now.

Edo Berger, a Hubble post-doctoral fellow at the Carnegie Observatories, is lead author of the first study that accurately pinpoints a short gamma-ray burst to an old dead galaxy, implicating a population of old neutron stars as the sources of these explosions. The study appears in the December 15, 2005, issue of Nature.

“We had no idea if they explode in nearby galaxies, or the farthest reaches of the universe, or even what kind of object was producing them,” stated Berger. “Now, after eluding us for years, we have finally found out what objects are giving rise to these explosions.” he added.

Because short gamma-ray bursts are fainter than the long bursts, they have been very difficult to localize until recently, with the advent of NASA’s Swift satellite and rapid follow-up by telescopes on the ground. Swift detects and observes gamma-ray bursts in multiple wavelengths and alerts astronomers who quickly point ground-based telescopes to catch the fading afterglow–the dying ember that glows for hours or days after the burst of gamma-rays.

In this study, Berger led a team that discovered and monitored the afterglow in radio, optical, and infrared wavelengths using telescopes at Carnegie’s Las Campanas Observatory in Chile and the Very Large Array in New Mexico.They homed in on a gamma-ray burst (GRB 050724) localized by Swift on July 24 and found that the emission came from a fairly close (3.5 billion light-years) old elliptical galaxy.

“When the images came in from the telescope in the middle of the night I was shocked,” said Berger.” We finally determined a precise position for a short burst, and it happened in the most unlikely of places, an old dead galaxy.” By the second night, the afterglow had completely faded away.

While long gamma-ray bursts result from the death of massive stars only a few million years old, the fact that the short burst occurred in an old elliptical galaxy, which has not formed new stars in several billion years, suggests that a completely different population of sources was at play. The objects giving rise to short bursts must be very old.

Theorists have long suspected that short gamma-ray bursts are the end product of a class of binary stars composed of two old neutron stars, or a neutron star and a black hole, which slowly approach each other as their orbit shrinks over hundreds of millions of years. This process results from the emission of gravitational waves, one of the major predictions of Einstein’s theory of general relativity. “Eventually, the two objects get so close together that they just shred each other apart in a cataclysmic explosion,” said Tsvi Piran, a theoretical astrophysicist from Hebrew University in Israel and a co-author on the paper.

Because GRB 050724 is the first short burst with detections across the electromagnetic spectrum, the study reveals that the energy produced in the burst was channeled out in narrow jets, similar to those observers have seen in many long GRBs. But the energy was one thousand times lower. “We have been simulating the explosions from neutron star collisions on computers for years” stated Stephan Rosswog, a professor of astronomy at the International University in Bremen, Germany. “It is exhilarating to finally compare our results to actual data, and I am happy to see that some of our predictions were validated,” he added.

The next stage in the study of short bursts is to locate and study a large number of these objects. “We have been studying the long GRBs for many years, and each one produces a new surprise,” said Berger. “I can’t wait to see what surprises the universe has in store for us with the short GRBs.”

In addition to Berger and Piran the international team that identified and researched the afterglow and host galaxy of the short GRB 050724 includes David Murphy and Eric Persson from Carnegie Observatories, Paul Price and Len Cowie from the University of Hawaii, Brad Cenko, Avishay Gal-Yam, Alicia Soderberg, Mansi Kasliwal, Doug Leonard, Brian Cameron, Shri Kulkarni, Dae-Sik Moon, Derek Fox, and Fiona Harrison from Caltech, Dale Frail from the National Radio Astronomy Observatory, Wojtek Krzeminski from Las Campanas Observatory, Brian Lee from the University of Toronto, Kathy Roth from the Gemini Observatory, Brian Schmidt, Joshua Rich, and Bruce Peterson from Mount Stromlo Observatory, and Bryan Penprase from Pomona College.

More information on Swift can be found at: http://swift.gsfc.nasa.gov/

Information about the Carnegie Observatories is at http://www.ociw.edu/

Gamma-ray burst research at Carnegie and Caltech is supported in part by funds from NASA. E.B. and A.G.Y. are supported by NASA through Hubble Fellowship grants awarded by the Space Telescope Science Institute, which is operated by AURA, Inc., for NASA. The VLA is operated by the National Radio Astronomy Observatory, a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

The Carnegie Observatories is part of the Carnegie Institution (www.CarnegieInstitution.org), which has been a pioneering force in basic scientific research since 1902. It is a private, nonprofit organization with six research departments throughout the U.S. Carnegie scientists are leaders in plant biology, developmental biology, astronomy, materials science, global ecology, and Earth and planetary science.