papers

Publications (10)

astro-ph2006

A Survey for Supernovae in Massive High-Redshift Clusters

Keren Sharon, A. Gal-Yam, D. Maoz +12

We describe our ongoing program designed to measure the SN-Ia rate in a sample of massive z=0.5-0.9 galaxy clusters. The SN-Ia rate is a poorly known observable, especially at high…

astro-ph2000

Thomson Thick X-ray Absorption in a Broad Absorption Line Quasar PG0946+301

S. Mathur, P. J. Green, N. Arav +14

We present a deep ASCA observation of a Broad Absorption Line Quasar (BALQSO) PG0946+301. The source was clearly detected in one of the gas imaging spectrometers, but not in any ot…

astro-ph2006

X-ray thermal coronae of galaxies in hot clusters -- ubiquity of embedded mini cooling cores

M. Sun, C. Jones, W. Forman +3

We present a systematic investigation of X-ray thermal coronae in 157 early-type galaxies and 22 late-type galaxies from a survey of 25 hot (kT>3 keV), nearby (z<0.05) clusters, ba…

astro-ph.GA2019

Deep and narrow CO absorption revealing molecular clouds in the Hydra-A brightest cluster galaxy

Tom Rose, A. C. Edge, F. Combes +20

Active galactic nuclei play a crucial role in the accretion and ejection of gas in galaxies. Although their outflows are well studied, finding direct evidence of accretion has prov…

astro-ph2005

A 70 kpc X-ray tail in the cluster A3627

M. Sun, C. Jones, W. Forman +3

We present the discovery of a 70 kpc X-ray tail behind the small late-type galaxy ESO137-001 in the nearby, hot (T=6.5 keV) merging cluster A3627, from both Chandra and XMM observa…

astro-ph.CO2012

Hundred Thousand Degree Gas in the Virgo Cluster of Galaxies

W. B. Sparks, J. E. Pringle, R. F. Carswell +6

The physical relationship between low-excitation gas filaments at ~10^4 K, seen in optical line emission, and diffuse X-ray emitting coronal gas at ~10^7 K in the centers of many g…

astro-ph.CO2009

Galaxy Cluster Astrophysics and Cosmology: Questions and Opportunities for the Coming Decade

S. T. Myers, C. Pfrommer, J. Aguirre +21

We are learning much about how structure forms, in particular how clusters as nodes in the cosmic web evolve and accrete matter, and about the physical processes within these objec…

astro-ph2001

Discovery of Ghost Cavities in Abell 2597's X-ray Atmosphere

B. R. McNamara, M. W. Wise, P. E. J. Nulsen +10

A Chandra image of the central 100 kpc of the Abell 2597 cluster of galaxies shows bright, irregular, X-ray emission within the central dominant cluster galaxy (CDG), and two low s…

astro-ph2005

An X-ray Galaxy Cluster Survey for Investigations of Dark Energy

Z. Haiman, S. Allen, N. Bahcall +34

The amount and nature of dark energy (DE) can be tightly constrained by measuring the spatial correlation features and evolution of a sample of ~ 100,000 galaxy clusters over the r…

astro-ph.CO2009

Discovery of CIV Emission Filaments in M87

W. B. Sparks, J. E. Pringle, M. Donahue +4

Gas at intermediate temperature between the hot X-ray emitting coronal gas in galaxies at the centers of galaxy clusters, and the much cooler optical line emitting filaments, yield…