RCS 043938-2904.9: A New Rich Cluster of Galaxies at [FORMULA][F]z=0.951[/F][/FORMULA]

2004 ◽  
Vol 617 (1) ◽  
pp. L17-L20 ◽  
Author(s):  
L. Felipe Barrientos ◽  
Michael D. Gladders ◽  
H. K. C. Yee ◽  
Leopoldo Infante ◽  
Erica Ellingson ◽  
...  
Keyword(s):  
Rich Cluster ◽  
Cluster Of Galaxies

C1 1358 + 6245 at Z = 0.32 - an X-ray selected, distant, rich cluster of galaxies

1991 ◽  
Vol 102 ◽  
pp. 1 ◽  
Author(s):  
Gerard A. Luppino ◽  
Brin A. Cooke ◽  
Ian M. McHardy ◽  
George R. Ricker
Keyword(s):  
Rich Cluster ◽  
X Ray ◽  
Cluster Of Galaxies

A Rich Cluster of Galaxies Near the Quasar B2 1335+28 atz= 1.1: Color Distribution and Star Formation Properties

2001 ◽  
Vol 546 (1) ◽  
pp. 604-604
Author(s):  
Ichi Tanaka ◽  
Toru Yamada ◽  
Alfonso Aragon‐Salamanca ◽  
Tadayuki Kodama ◽  
Takamitsu Miyaji ◽  
...  
Keyword(s):  
Star Formation ◽  
Rich Cluster ◽  
Color Distribution ◽  
Cluster Of Galaxies

scholarly journals ASCA Observations of the Abell 496 Cluster of Galaxies

1998 ◽  
Vol 188 ◽  
pp. 304-305
Author(s):  
I. Hatsukade ◽  
J. Ishizaka ◽  
M. Yamauchi ◽  
K. Takagishi
Keyword(s):  
Mass Flow Rate ◽  
Chemical Evolution ◽  
Mass Flow ◽  
Relative Abundance ◽  
Flow Rate ◽  
Metal Distribution ◽  
Rich Cluster ◽  
Cooling Flow ◽  
Evolution Of Galaxies ◽  
Cluster Of Galaxies

The metal in the intracluster medium (ICM) has been ejected or stripped from galaxies. Thus measurements of the metal distribution and the relative abundance of elements, in particular Si/Fe, are important to study the evolution of galaxies, as well as to study the chemical evolution of the ICM. We present the results from ASCA observations of Abell 496 cluster of galaxies. A496 is a nearby rich cluster with a central cD galaxy. At the redshift z=0.0327 of A496, 1 arcmin is 53kpc, where we assumed H0 = 50kms−1Mpc−1, q0 = 0.5. A496 is known as a cooling flow cluster. Edge and Stewart (1991) obtained the mass flow rate of and the cooling radius of 177 ± 52kpc.

scholarly journals Optical–infrared studies of the rich cluster of galaxies Abell 370 at z = 0.37

1991 ◽  
Vol 248 (1) ◽  
pp. 128-138 ◽  
Author(s):  
Alfonso Aragón-Salamanca ◽  
Richard S. Ellis ◽  
Ray M. Sharples
Keyword(s):  
Rich Cluster ◽  
Cluster Of Galaxies ◽  
Infrared Studies ◽  
The Rich

A study of the rich cluster of galaxies A 119

1993 ◽  
Vol 105 ◽  
pp. 788 ◽  
Author(s):  
Daniel Fabricant ◽  
Michael Kurtz ◽  
Margaret Geller ◽  
Ann Zabludoff ◽  
Peter Mack ◽  
...  
Keyword(s):  
Rich Cluster ◽  
Cluster Of Galaxies ◽  
The Rich

scholarly journals The rich cluster of galaxies A348

1990 ◽  
Vol 242 (2) ◽  
pp. 112-119 ◽  
Author(s):  
S. J. C. Millington ◽  
J. V. Peach
Keyword(s):  
Rich Cluster ◽  
Cluster Of Galaxies ◽  
The Rich

Evidence of a Large Scale Magnetic Field in the Coma - A1367 Supercluster

1990 ◽  
Vol 140 ◽  
pp. 492-494 ◽  
Author(s):  
G. Giovannini ◽  
K.-T. Kim ◽  
P. P. Kronberg ◽  
T. Venturi
Keyword(s):  
Magnetic Field ◽  
Large Scale ◽  
Galaxy Cluster ◽  
Coma Cluster ◽  
Rich Cluster ◽  
Cluster Of Galaxies ◽  
Large Scale Magnetic Field

The Coma cluster is a rich cluster of galaxies nested in an even larger supercluster of galaxies. The plane of the supercluster appears to be defined by the Coma cluster itself and another galaxy cluster, Abell 1367, that lies about 40 Mpc (H0 = 75 Mpc km−1s−1 (≡h75)) farther west (Tifft and Gregory 1976).

scholarly journals BeppoSAX observation of the rich cluster of galaxies Abell 85

2001 ◽  
Vol 368 (2) ◽  
pp. 440-450 ◽  
Author(s):  
G. B. Lima Neto ◽  
V. Pislar ◽  
J. Bagchi
Keyword(s):  
Rich Cluster ◽  
Cluster Of Galaxies ◽  
The Rich

scholarly journals Intermediate-band photometry of a rich cluster of galaxies: A2218

2001 ◽  
Vol 369 (3) ◽  
pp. 750-757 ◽  
Author(s):  
K. Rakos ◽  
D. Dominis ◽  
S. Steindling
Keyword(s):  
Rich Cluster ◽  
Intermediate Band ◽  
Cluster Of Galaxies
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