The Chandra exhibit booth (Credit: CXC) |
The Chandra exhibit booth. (Credit: CXC) |
The backlit poster in the Chandra exhibit booth. (Credit: CXC) |
The plasma display in the Chandra exhibit booth. (Credit: CXC) |
CIAO demos and software assistance at the Chandra exhibit booth. (Credit: CXC) |
| Session: Supernova Remnants
Poster Title: Chandra Observations of SNR1987A |
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Chandra observes aging and exploding stars as well as young stars. In this paper the authors discuss the results of monitoring a supernova remnant using Chandra. This supernova remnant is what remains of a star that exploded in 1987. Using Chandra data, the authors have measured the ongoing expansion rate of material from the explosion. | |
| Session: Chandra Observations of Nearby Galaxies
Poster Title: New X-ray Featurs in the Elliptical Galaxy NGC 4472 |
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Chandra can look out beyond our own galaxy, and this poster presents observations of a nearby galaxy called NGC 4472. These observations show features in this galaxy that may indicate that it has collided with other nearby galaxies. And, other features in the X-ray data provide clues about the history of supernovae explosions within this galaxy. | |
| Session: A Multiwavelength Look
Poster Title: Diffuse Emission in the Nucleus of M31 |
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The galaxy M31 is one of our galaxy's closest galactic neighbors. This poster reports on Chandra observations that help to more precisely determine the temperature of the hot gas that surrounds the core of M31. | |
| Session: Active Galactic Nuclei - Surveys
Poster Title: Chandra Observations of the Radio Jets in a Sample of Quasars |
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Observations with Chandra often result in new discoveries, as did those reported here: four new X-ray jets were discovered. These jets emanate from the cores of active galaxies. | |
| Session: Galaxy Clusters and Mergers
Poster Title: Chandra Observations of the Disruption of the Cool Core in Abell 133 |
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Like stars that are drawn together by gravity into galaxies, galaxies are also drawn together into groups. Chandra can observe these galaxy clusters, and this paper reports on observations made of the core of a cluster called Abell 133. This core exhibits a filamentary structure of an as-yet unknown nature. | |
Chandra press conference. (Credit: CXC) |