Chandra scores a double bonus with a distant quasar
CHANDRA X-RAY CENTER NEWS RELEASE
Posted: February 8, 2002
Two discoveries from a distant quasar -- an enormous X-ray jet and an X-ray shadow cast by an intervening galaxy -- are giving astronomers using NASA's Chandra X-ray Observatory cause to be doubly excited. These two independent results reveal information about a supermassive black hole at the center of the quasar as well as the amount of oxygen in a distant galaxy billions of years ago.
"The X-rays from the jet are likely due to the collision of microwave photons left over from the Big Bang with a high-energy beam of particles," said Aneta Siemiginowska of the Harvard-Smithsonian Center for Astrophysics in Cambridge, MA, lead author on a paper which will appear in the May 10, 2002 issue of the Astrophysical Journal. "The intensity of these microwaves today is much less than it was 10 billion years ago, due to the expansion of the universe."
Chandra observations of quasar PKS 1127-145 demonstrate that scientists can image these jets even though they are billions of light years away. Studies of these extraordinarily large structures will allow astronomers to test models for quasars and the supermassive black holes that power them.
The length of the jet and the prominent knots of X-ray emission observed suggest that the activity in the vicinity of the central supermassive black hole is long-lived but maybe intermittent, perhaps due to the mergers of other galaxies with the host galaxy.
Atoms of various elements in this galaxy absorb some of the X-rays, yielding a dimming of the quasar's X-rays. In a similar way, when our body is X-rayed, our bones produce an X-ray shadow. In this case, the quasar acts as the X-ray machine. By measuring the amount of absorption, astronomers were able to estimate that the intervening galaxy contained only about 20 percent as much oxygen as our Milky Way Galaxy has now. These observations will give astronomers insight into how the oxygen supply of galaxies is built up over the eons.
"We are looking at a galaxy at about the time in the history of the universe when our sun formed," said Jill Bechtold of the University of Arizona, the lead author on another paper in the November 20, 2001 issue of The Astrophysical Journal that describes these results. "It's intriguing that this galaxy had only about 1/5 of the oxygen that we now measure for typical stars in our Galaxy."
Scientists believe that elements such as oxygen, silicon and sulfur are dispersed into the galaxy primarily by the explosion of massive stars. As galaxies age, they become more enriched in oxygen and other elements necessary for life. Using the fact that the light travel time from distant galaxies can range from hundreds of millions to billions of years, astronomers can study the rate of this enrichment.
"X-ray observations are especially important for this study," emphasized Bechtold. "They provide a direct measurement of the abundance of oxygen atoms without the complications of dust and other factors that make the interpretation of optical and ultraviolet observations difficult."