Wong, Ka-Wah, Sarazin, Craig L., Blanton, Elizabeth L., Reiprich, Thomas H.
We present a detailed analysis of the XMM-Newton and Chandra observations of Abell 2626 focused on the X-ray and radio interactions. Within the region of the radio mini-halo (~70 kpc), there are...
Ka-wah Wong, Craig L. Sarazin, Elizabeth L. Blanton, Thomas H. Reiprich
We present a detailed analysis of the XMM-Newton and Chandra observations of Abell 2626 focused on the X-ray and radio interactions. Within the region of the radio mini-halo ( ∼ 70 kpc), there are...
Elizabeth L. Blanton, Craig L. Sarazin, Brian R. Mcnamara, Michael W. Wise
We present a Chandra observation of Abell 2052, a cooling flow cluster with a central cD that hosts the complex radio source 3C 317. The data reveal "holes " in the X-ray emission...
DIFFUSE GAS AND LMXBS IN THE CHANDRA OBSERVATION OF THE S0 GALAXY NGC 1553 (2007)
Elizabeth L. Blanton, Craig L. Sarazin, Jimmy A. Irwin
We have spatially and spectrally resolved the sources of X-ray emission from the X-ray faint S0 galaxy NGC 1553 using an observation from the Chandra X-ray Observatory. The majority (70%) of the...
Chandra Observation of the Cluster Environment of a WAT Radio Source in Abell 1446 (2007)
Douglass, E. M., Blanton, Elizabeth L., Clarke, T. E., Sarazin, Craig L., Wise, Michael
Wide-angle tail (WAT) radio sources are often found in the centers of galaxy clusters where intracluster medium (ICM) ram pressure may bend the lobes into their characteristic C-shape. We examine the...
The Complex Cooling Core of Abell 2029: Radio and X-ray Interactions (2004)
Clarke, Tracy E., Blanton, Elizabeth L., Sarazin, Craig L.
We present an analysis of Chandra observations of the central regions of the cooling flow cluster Abell 2029. We find a number of X-ray filaments in the central 40 kpc, some of which appear to be...
Blanton, Elizabeth L., Sarazin, Craig L., McNamara, Brian R., Clarke, T. E.
We present a Chandra observation of the cooling flow cluster Abell 262. Spectral fits show that the intracluster medium (ICM) in A262 cools by a factor of three from 2.7 keV to 0.9 keV at the cluster...
The Interaction of Radio Sources and X-ray-Emitting Gas in Cooling Flows (2004)
Recent observations of the interactions between radio sources and the X-ray-emitting gas in cooling flows in the cores of clusters of galaxies are reviewed. The radio sources inflate bubbles in the...
A Taxonomy of Extended Radio Sources in Clusters of Galaxies (2003)
Kempner, Joshua C., Blanton, Elizabeth L., Clarke, Tracy E., Ensslin, Torsten A., Johnston-Hollitt, Melanie, Rudnick, Lawrence
At the request of the conference attendees, we have compiled a classification of extended radio sources in clusters. These range from scales of tens of parsecs to over a megaparsec in scale, and...
Cooling of X-ray Emitting Gas by Heat Conduction in the Center of Cooling Flow Clusters (2003)
Soker, Noam, Blanton, Elizabeth L., Sarazin, Craig L.
We study the possibility that a large fraction of the gas at temperatures of \~10^7 K in cooling flow clusters cools by heat conduction to lower temperatures, rather than by radiative cooling. We...
Low Mass X-ray Binaries and Globular Clusters in Early-Type Galaxies (2003)
Sarazin, Craig L., Kundu, Arunav, Irwin, Jimmy A., Sivakoff, Gregory R., Blanton, Elizabeth L., Randall, Scott W.
(Abridged) A high fraction of the Low Mass X-ray Binaries (LMXBs) in early-type galaxies are associated with globular clusters (GCs). Here, we discuss the correlations between LMXBs and GCs in a...
Chandra Observations of the Central Region of Abell 3112 (2003)
Takizawa, Motokazu, Sarazin, Craig L., Blanton, Elizabeth L., Taylor, Greg B.
We present the results of a {\it Chandra} observation of the central region of Abell 3112. This cluster has a powerful radio source in the center and was believed to have a strong cooling flow. The...
Blanton, Elizabeth L., Gregg, Michael D., Helfand, David J., Becker, Robert H., White, Richard L.
Using a combination of near-infrared and optical photometry, along with multi-object spectroscopy, we have confirmed the existence of a high-redshift cluster of galxies at z = 0.96. The cluster was...
Chandra Observation of the Cooling Flow Cluster Abell 2052 (2002)
Blanton, Elizabeth L., Sarazin, Craig L., McNamara, Brian R.
We present an analysis of the Chandra X-ray observation of Abell 2052, including large scale properties of the cluster as well as the central region which includes the bright radio source, 3C 317. We...
Hot Bubbles in Cooling Flow Clusters (2002)
Soker, Noam, Blanton, Elizabeth L., Sarazin, Craig L.
As more cooling flow clusters of galaxies with central radio sources are observed with the Chandra and XMM-Newton X-ray Observatories, more examples of "bubbles" (low-emission regions in the X-ray...
Blanton, Elizabeth L., Sarazin, Craig L., McNamara, Brian R., Wise, Michael W.
We present a Chandra observation of Abell 2052, a cooling flow cluster with a central cD that hosts the complex radio source 3C 317. The data reveal ``holes'' in the X-ray emission that are...