J/A+AS/113/451           Superclusters of galaxies      (Kalinkov+ 1995)

Superclusters of galaxies. I. The catalog Kalinkov M., Kuneva I. <Astron. Astrophys. Suppl. Ser. 113, 451 (1995)> =1995A&AS..113..451K 1995A&AS..113..451K (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy Keywords: (cosmology:) large-scale structure of Universe - Galaxies: clusters of Description: All rich clusters of galaxies from Abell and ACO catalogs are examined to find superclusters of galaxies. Measured as well as estimated redshift of the clusters is used and the study is in the redshift space. The searching procedure is general and is applicable not only to clusters of galaxies, but also to galaxies to find groups. The number of detected superclusters of galaxies for space density enhancement f=10, 20, 40, 100, 200 and 400 is 893. The enhancement is above a local density defined for a sphere with radius 100 Mpc around each cluster. Kinematical and dynamical properties for superclusters, containing at least one cluster with measured redshift and generally located up to distance 627 Mpc (z = 0.20) with |b|>40deg are given. A detailed comparison with other catalogs is carried out. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2 104 603 Superclusters of galaxies with multiplicity ν≥2 (at least one member with measured redshift) table5 46 207 Characteristics of superclusters table8 16 40 E27 - Horologium-Reticulum supercluster table9 17 29 E80 - Shapley concentration table10 18 21 E6 - Pisces-Cetus supercluster table11 70 116 Identification of superclusters -------------------------------------------------------------------------------- Table 6: P2 and P4, f=10; SC431; n100 is the number of clusters in a sphere with radius of 100Mpc, centered on the running cluster; r is the distance from the supercluster centre to each member. ---------------------------------------------------------------------------- nu A-cluster n100 r (Mpc) D100 (Mpc-3) ---------------------------------------------------------------------------- 1 1177 7.7 2 999 40 16.4 9.55E-06 3 1016 40 17.5 9.55E-06 4 1185 18.2 5 1142 45 18.3 1.07E-05 6 1267 19.3 D6 = 1.99E-04 Mpc-3 ---------------------------------------------------------------------------- 7 1257 32.0 D6+1 = 5.10E-05 1 1142 8.0 2 1016 16.2 3 1139 42 17.2 1.00E-05 D3 = 1.412E-04 ---------------------------------------------------------------------------- 4 999 19.2 D3+1 = 1.341E-04 1 1267 42 5.9 1.00E-05 2 1185 39 6.7 9.31E-06 3 1257 40 10.8 9.55E-06 4 1228 36 13.2 8.59E-06 5 1177 43 14.7 1.03E-05 D5 = 3.77E-04 ---------------------------------------------------------------------------- 6 1314 34.7 D5+1 = 3.43E-05 ---------------------------------------------------------------------------- Table 7: Superclusters from Einasto et al. 1994 (E), which are not found in this paper ------------------------- E ------------------------- 1 22 45 76. 104. 2 26 49 77. 105. 4 28 50 79. 107. 5 30 65 85. 114. 11 34-39 68 94. 117. 16 42 69 99. 120. 21 44 71 103. 121. ------------------------- Byte-by-byte Description of file: table2 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 --- SC Supercluster of galaxies number 6- 7 I2 --- nu []? Supercluster multiplicity 9- 11 I3 --- f1 []? Space density enhancement(first value) 12 A1 --- "-" [-] Separation label 13- 15 I3 --- f2 []? Space density enhancement 17- 20 I4 --- Clust1 A-cluster (1) 21 A1 --- n_Clust1 [z] z means measured redshift (2) 23- 26 I4 --- Clust2 []? A-cluster (1) 27 A1 --- n_Clust2 [z] z means measured redshift (2) 29- 32 I4 --- Clust3 []? A-cluster (1) 33 A1 --- n_Clust3 [z] z means measured redshift (2) 35- 38 I4 --- Clust4 []? A-cluster (1) 39 A1 --- n_Clust4 [z] z means measured redshift (2) 41- 42 I2 h RAh []? Right ascension (1950) 44- 47 F4.1 min RAm []? Right ascension (1950) 49 A1 --- DE- Declination sign 50- 51 I2 deg DEd []? Declination (1950) 53- 54 I2 arcmin DEm []? Declination (1950) 56- 60 F5.1 deg GLAT []? Galactic latitude 62- 64 I3 Mpc Dist []? Mean luminosity distance 66- 69 F4.1 Mpc DRA []? Maximum supercluster size along right ascension 71- 74 F4.1 Mpc DDE []? Maximum supercluster size along declination 76- 79 F4.1 Mpc DDist []? Maximum supercluster size along mean luminosity distance 81- 84 F4.1 Mpc Rnu []? Separation from the supercluster centre to the most distant member 86- 89 F4.1 Mpc Rnu+1 []? Separation between supercluster centre and the nearest neighbour cluster out of the supercluster 91- 97 E7.1 Mpc-3 Dens []? Ratio of the supercluster density to the mean local density, defined within a sphere of 100 Mpc radius 99-103 F5.1 10+14solMass Mass []? Supercluster mass -------------------------------------------------------------------------------- Note (1): Abell 1958 and Abell et al. 1989 Note (2): otherwise multiple regression estimate is used -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 --- SC Supercluster of galaxies number 6- 7 I2 --- nu []? Supercluster multiplicity 9- 11 I3 --- f1 []? Space density enhancement (first value) 12 A1 --- "-" [-] Separation label 13- 15 I3 --- f2 []? Space density enhancement 17- 20 F4.1 Mpc MaxDist Maximum pair distance in superclusters 22- 25 F4.1 Mpc MinDist Minimum pair distance in superclusters 27- 30 F4.1 Mpc HarRad Mean harmonic radius 32- 35 F4.1 Mpc PairDist Mean pair separation 37- 40 I4 km/s Vel []? 3D Velocity dispersion 42- 46 F5.2 --- Crt []? Crossing time in units of Hubble time -------------------------------------------------------------------------------- Byte-by-byte Description of file: table8 table9 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 5 I4 --- Cluster []? Abell numbers (Abell 1958 and Abell et al. 1989) for the corresponding supercluster from Einasto et al. 1994 (E-supercluster) 7 A1 --- n_SC [A] When 'A' Abell cluster additional for E-supercluster, but member of the other supercluster 8- 11 I4 --- SC []? Supercluster of galaxies number 13 A1 --- n_Z-number When 'A' Abell cluster additional for E-supercluster, but member of the other supercluster 14- 17 I4 --- Z-number []? Zucca et al. 1993 identification number -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 5 I4 --- Cluster []? Abell numbers (Catalog VII/110) for the corresponding supercluster from Einasto et al. 1994 (E-supercluster) 7 A1 --- n_SC [A] When 'A' Abell cluster additional for E-supercluster, but member of the other supercluster 8- 11 I4 --- SC []? Supercluster of galaxies number 13 I1 --- Z-number []? Zucca et al. 1993 identification number 15- 16 I2 --- P-number []? Postman et al. 1992 identification number 18 I1 --- W-number []? West 1989 identification number -------------------------------------------------------------------------------- Byte-by-byte Description of file: table11 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 --- SC []? Supercluster of galaxies number 6- 8 I3 --- f1 []? Space density enhancement (first value) 9 A1 --- "-" [-] Separation label 10- 12 I3 --- f2 []? Space density enhancement 14 I1 --- nu []? Supercluster multiplicity 16- 70 A55 --- Identif Identification (1) -------------------------------------------------------------------------------- Note (1): E: Einasto et al. 1994 Z: Zucca et al. 1993 P: Postman et al. 1992 W: West 1989 B: Bahcall et al. 1984 T: Thuan 1980 -------------------------------------------------------------------------------- See also: VII/110 : Abell's catalog (=1958ApJS....3..211A 1958ApJS....3..211A) References: Abell G.O. =1958ApJS....3..211A 1958ApJS....3..211A Abell G.O., Corwin H.G., Olowin R.P. =1989ApJS...70....1A 1989ApJS...70....1A Bahcall N.A. and Soneira R.M. =1984ApJ...277...27B 1984ApJ...277...27B Einasto M., Einasto J., Tago E., Dalton G.B., Andernach H. =1994MNRAS.269..301E 1994MNRAS.269..301E Postman M., Huchra J.P., Geller M.J. =1992ApJ...384..404P 1992ApJ...384..404P Thuan T.X. 1980, "The Large-Scale Distribution of Galaxies", in: Balian R., Audouze J., Schramm D.N. (eds.) Physical Cosmology. North-Holland, Amsterdam, p. 277; West M.J., =1989ApJ...347..610W 1989ApJ...347..610W Zucca E., Zamorani G., Scaramella R., Vettolani G., =1993ApJ...407..470Z 1993ApJ...407..470Z
(End) Simona Mei [CDS] 07-Jun-1995
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line