The Cold Gas in Cluster Cores – so much progress in the Chandra era

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The Cold Gas in Cluster Cores – so much progress in the Chandra era Alastair Edge (Durham University) and many collaborators

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The Cold Gas in Cluster Cores – so much progress in the Chandra era. Alastair Edge (Durham University) a nd many collaborators. Cold?. This conference is primarily focused (rightly) on the X-ray regime so I should just define the parameters for this talk! - PowerPoint PPT Presentation

Transcript of The Cold Gas in Cluster Cores – so much progress in the Chandra era

The Cold Gas in Cluster Cores so much progress in the Chandra era

The Cold Gas in Cluster Cores so much progress in the Chandra eraAlastair Edge(Durham University)and many collaboratorsCold?This conference is primarily focused (rightly) on the X-ray regime so I should just define the parameters for this talk!I regard cold as gas with a temperature of


Tidal Debris in Galaxy Cluster Cores

Tidal Debris in Galaxy Cluster Cores

RGS observations of cool gas in cluster cores

RGS observations of cool gas in cluster cores

Enigma, Sun Grid Engine (SGE), and the Joint High ...• Cluster software server (AMD Opteron, 8-cpu cores, 8 GB) – Provides software (apps) over the network for the cluster nodes

Enigma, Sun Grid Engine (SGE), and the Joint High ...• Cluster software server (AMD Opteron, 8-cpu cores, 8 GB) – Provides software (apps) over the network for the cluster nodes

A 1.15 TOPS/W, 16-Cores Parallel Ultra-Low Power Cluster ...

A 1.15 TOPS/W, 16-Cores Parallel Ultra-Low Power Cluster ...

HIGH-RESOLUTION CHANDRA X-RAY IMAGING AND …townsend/resource/publications/offprints/sorie... · HIGH-RESOLUTION CHANDRA X-RAY IMAGING AND SPECTROSCOPY OF THE ORIONIS CLUSTER Stephen

HIGH-RESOLUTION CHANDRA X-RAY IMAGING AND …townsend/resource/publications/offprints/sorie... · HIGH-RESOLUTION CHANDRA X-RAY IMAGING AND SPECTROSCOPY OF THE ORIONIS CLUSTER Stephen

Pi‘sToGo · 1. Like a Laptop 2. Actually a Cluster 3. Inner workings of the Cluster Design . SIGCSE&2015& 3 › < $500 * › 5 Nodes › 5-20 Cores › 10/100Mbps › 2.5-5 GB of

Pi‘sToGo · 1. Like a Laptop 2. Actually a Cluster 3. Inner workings of the Cluster Design . SIGCSE&2015& 3 › < $500 * › 5 Nodes › 5-20 Cores › 10/100Mbps › 2.5-5 GB of

The Cold Gas in Cluster Cores – so much progress in the Chandra era Alastair Edge (Durham University) and many collaborators.

The Cold Gas in Cluster Cores – so much progress in the Chandra era Alastair Edge (Durham University) and many collaborators.

Cores, cores, everywhere

Cores, cores, everywhere

High Performance Computing with the Cluster „Elwetritsch - II · High Performance Computing with the Cluster ... compute nodes ... more cores in total, ...

High Performance Computing with the Cluster „Elwetritsch - II · High Performance Computing with the Cluster ... compute nodes ... more cores in total, ...

Heating in cluster cool cores Mateusz Ruszkowski University of Michigan.

Heating in cluster cool cores Mateusz Ruszkowski University of Michigan.

M7: Next Generation SPARC Hotchips 26 – August 12, …swisdev.oracle.com/_files/M7_Preso.pdf · SPARC T4 § 8 S3 Cores § 4MB ... • 4 SPARC Cores Per Cluster

M7: Next Generation SPARC Hotchips 26 – August 12, …swisdev.oracle.com/_files/M7_Preso.pdf · SPARC T4 § 8 S3 Cores § 4MB ... • 4 SPARC Cores Per Cluster

The cluster scaling relations observed by Chandra

The cluster scaling relations observed by Chandra

GH2005 Gas Dynamics in Clusters II Craig Sarazin Dept. of Astronomy University of Virginia A85 Chandra (X-ray) Cluster Merger Simulation.

GH2005 Gas Dynamics in Clusters II Craig Sarazin Dept. of Astronomy University of Virginia A85 Chandra (X-ray) Cluster Merger Simulation.

UPPMAX Introduction...+ Snowy (old Milou): ~ 200 nodes à 16 cores (128, 256 & 512 GB RAM) Bianca: 200 nodes à 16 cores (128, 256 & 512 GB RAM) - virtual cluster >12 PB fast parallel

UPPMAX Introduction...+ Snowy (old Milou): ~ 200 nodes à 16 cores (128, 256 & 512 GB RAM) Bianca: 200 nodes à 16 cores (128, 256 & 512 GB RAM) - virtual cluster >12 PB fast parallel

A CHANDRA X-RAY STUDY OF THE DENSE GLOBULAR …cxc.harvard.edu/cal/Acis/Papers/heinke.pdfWe report a Chandra ACIS-I observation of the dense globular cluster Terzan 5. The previously

A CHANDRA X-RAY STUDY OF THE DENSE GLOBULAR …cxc.harvard.edu/cal/Acis/Papers/heinke.pdfWe report a Chandra ACIS-I observation of the dense globular cluster Terzan 5. The previously

HST Observations of Galactic Globular Cluster Cores. II ... · the dispersion in color due to photometric errors along the RGB (for 17

HST Observations of Galactic Globular Cluster Cores. II ... · the dispersion in color due to photometric errors along the RGB (for 17

((Title)) · Web viewand [MnIII 4 LnIII 4 (C[4]) 4] cluster cores in Figures 1A and 1B respectively.[9b,c] Analysis of our library of cluster types and conditions employed has allowed

((Title)) · Web viewand [MnIII 4 LnIII 4 (C[4]) 4] cluster cores in Figures 1A and 1B respectively.[9b,c] Analysis of our library of cluster types and conditions employed has allowed

MagAmp cores MagAmp Cores

MagAmp cores MagAmp Cores

Main-Cluster XIS0XIS1XIS3 Weighted mean Chandra Figure 2 : XIS spectra of the main-cluster XIS0 0.4-10keV Main-Cluster Sub-Cluster Search for Bulk Motion.

Main-Cluster XIS0XIS1XIS3 Weighted mean Chandra Figure 2 : XIS spectra of the main-cluster XIS0 0.4-10keV Main-Cluster Sub-Cluster Search for Bulk Motion.

EPIC Chandra Cross Calibration with the Perseus Cluster · Cross Cal with Clusters • Has enjoyed some success • Perseus is the brightest cluster in the X - ray sky • Lots of

EPIC Chandra Cross Calibration with the Perseus Cluster · Cross Cal with Clusters • Has enjoyed some success • Perseus is the brightest cluster in the X - ray sky • Lots of