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BU Astrophysicist Leads Team That Discovers “Sloshing” Gas in Galaxy Cluster

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X-ray: NASA/CXC/BU/E.Blanton; Optical: ESO/VLT

Composite X-ray (blue) / optical (orange) image of the cluster of galaxies Abell 2052. The hot gas in the galaxy cluster Abell 2052 is being sloshed back and forth like wine in a glass. The sloshing was set in motion when a small cluster smashed into the larger central one. The large spiral structure on the outside of the image was also caused by that off center collision. Sloshing of hot gas like this can affect how the giant elliptical galaxy and its supermassive black hole at the center grow.

Boston—Boston University astrophysicist Elizabeth Blanton led a team of researchers in the discovery of vast clouds of hot gas "sloshing" in Abell 2052, a galaxy cluster located about 480 million light years from Earth. The scientists are studying the hot (30 million degree) gas using X-ray data from NASA's Chandra X-ray Observatory. The team’s findings were first published in the August 20, 2011 issue of The Astrophysical Journal.

Blanton, assistant professor of astronomy at Boston University, is the project’s principal investigator and the paper’s lead writer. She and her colleagues observed that, like wine in a glass, vast clouds of hot gas are sloshing back and forth in Abell 2052. X-ray data from NASA's Chandra X-ray Observatory shows the hot gas in this dynamic system, and optical data from the Very Large Telescope shows the galaxies. The hot, X-ray bright gas has an average temperature of about 30 million degrees.

“The majority of the mass that we can directly observe in a cluster of galaxies emits in the X-ray, rather than the visible light we can see with our eyes. This X-ray emission reveals important physics at play in these objects, significant to the formation and evolution of galaxies. In this cluster, we have a spectacular combination of the large-scale “sloshing” spiral and central “bubbles” related to outbursts from a supermassive black hole,” Blanton explained.

A huge spiral structure in the hot gas - spanning almost a million light years - is seen around the outside of the image, surrounding a giant elliptical galaxy at the center. This spiral was created when a small cluster of galaxies smashed into a larger one that surrounds the central elliptical galaxy.

As the smaller cluster approached, the dense hot gas of the central cluster was attracted to it by gravity. After the smaller cluster passed the cluster core, the direction of motion of the cluster gas reversed and it traveled back towards the cluster center. The cluster gas moved through the center again and "sloshed" back and forth, similar to wine sloshing in a glass that was jerked sideways. The sides of the glass push the wine back to the center, whereas in the cluster the gravitational force of the matter in the clusters pulls it back. The sloshing gas ended up in a spiral pattern because the collision between the two clusters was off-center.

This type of sloshing in Abell 2052 has important physical implications. First, it helps push some of the more dense, cooler gas located in the center of the cluster -- where temperatures are only about 10 million degrees -- farther away from the core. This helps prevent further cooling of this gas in the core and could limit the amount of new stars being formed in the central galaxy. Sloshing motions like those seen in Abell 2052 also redistribute heavy elements, like iron and oxygen, which are forged in supernova explosions. These elements are used in the future generations of stars and planets and are necessary for life as we know it.

Chandra's observation of Abell 2052 was particularly long, lasting more than a week. Such a deep observation was necessary to detect all of the details in this image. Even then, processing to emphasize more subtle features was necessary to reveal the outer spiral structure.

In addition to the large-scale spiral feature, the deep Chandra observation reveals exquisite detail in the cluster center related to outbursts from the central supermassive black hole. The Chandra data show clear bubbles evacuated by material blasted away from the black hole, which are surrounded by dense, bright, cool rims. As with the sloshing, this activity helps prevent cooling of the gas in the cluster's core, setting limits on the growth of the giant elliptical galaxy and its supermassive black hole.

Blanton's primary field of research is clusters of galaxies, and she uses these objects to study galaxy formation and evolution as well as cosmology. She studies data taken at many wavelengths, but has a particular fondness for X-ray observations with Chandra. The full author list for The Astrophysical Journal paper is: Elizabeth Blanton of Boston University in Boston, MA; Scott Randall of the Harvard-Smithsonian Center for Astrophysics in Cambridge, MA; Tracy Clarke of the Naval Research Laboratory in Washington DC; Craig Sarazin of the University of Virginia in Charlottesville, VA; Brian McNamara of the University of Waterloo in Waterloo, Canada; Edmund Douglass of Boston University and Michael McDonald of the University of Maryland, College Park, MD.

About Boston University—Founded in 1839, Boston University is an internationally recognized private research university with more than 30,000 students participating in undergraduate, graduate, and professional programs. As Boston University’s largest academic division, the College and Graduate School of Arts & Sciences is the heart of the BU experience with a global reach that enhances the University’s reputation for teaching and research.

Contact information for the authors:

Dr. Elizabeth Blanton
Astronomy Department
Boston University
725 Commonwealth Avenue
Boston, MA 02215

Phone: 617-353-2633 or 2625
Email: eblanton@bu.edu

Dr. Elizabeth Blanton | Quelle: Newswise Science News
Weitere Informationen: www.bu.edu

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