ACO 1079 , the SIMBAD biblio

ACO 1079 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST08:26:09


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Title First 3 Authors
1971ApJS...23..371S 2711 51 Rectangular coordinates of rich clusters of galaxies on the Palomar Sky Survey charts. SASTRY G.N. and ROOD H.J.
1984AJ.....89.1487S 1087 42 Morphological classification (revised RS) of Abell clusters in D=5 and an analysis of observed correlations. STRUBLE M.F. and ROOD H.J.
1987ApJS...63..555S viz 2712 116 A catalog of morphological properties of the 2712 Abell clusters. STRUBLE M.F. and ROOD H.J.
1988AJ.....96.1534S 411 6 Position-angle statistics of the brightest binary galaxies in Abell clusters. STRUBLE M.F.
1989ApJS...70....1A viz 5256 1561 A catalog of rich clusters of galaxies. ABELL G.O., CORWIN H.G.Jr and OLOWIN R.P.
1995A&AS..113..451K viz 1283 14 Superclusters of galaxies. I. The catalog. KALINKOV M. and KUNEVA I.
2002MNRAS.331..333P 2 14 94 The Las Campanas/AAT Rich Cluster Survey - II. The environmental dependence of galaxy colours in clusters at z ∼0.1. PIMBBLET K.A., SMAIL I., KODAMA T., et al.
2004MNRAS.347..137P 40   K                 2 19 Intercluster Filaments of Galaxies Programme: pilot study survey and results. PIMBBLET K.A. and DRINKWATER M.J.
2005MNRAS.358..256P 1 8 24 A new algorithm for the detection of intercluster galaxy filaments using galaxy orientation alignments. PIMBBLET K.A.
2005MNRAS.359..272C 7 8 173 Intercluster filaments in a ΛCDM Universe. COLBERG J.M., KRUGHOFF K.S. and CONNOLLY A.J.
2006MNRAS.366..645P viz 6439 72 The Las Campanas/Anglo-Australian Telescope Rich Cluster Survey - III. Spectroscopic studies of X-ray bright galaxy clusters at z∼ 0.1. PIMBBLET K.A., SMAIL I., EDGE A.C., et al.
2005PASA...22..136P 37           X         1 16 10 Pulling out threads from the cosmic tapestry: Defining filaments of galaxies. PIMBBLET K.A.
2010MNRAS.401.2257M 39           X         1 8 18 Probing the cosmic web: intercluster filament detection using gravitational lensing. MEAD J.M.G., KING L.J. and McCARTHY I.G.

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