Compact groups of galaxies (CGs) from the SDSS Data Release 6

• Authors: Xin-Fa Deng , Ji-Zhou He , Xin-sheng Ma , Peng Jiang , Xiao-Xun Tang
• Languages of publication: EN

Abstracts

EN

From the volume-limited MAIN galaxy sample of the SDSS Data Release 6 (SDSS6), we have identified 1298 compact groups of galaxies (CGs) at the neighbourhood radius of R = 1.2 Mpc by three-dimensional cluster analysis. In order to compile the CG catalog, we also estimated velocity dispersion, virial radius, virial mass and crossing time of CGs. In addition, our results show that properties of galaxies may not correlate with merging frequencies.

Keywords

EN

galaxy; fundamental parameters; large scale

• Publisher: De Gruyter Open
• Journal: Open Physics
• Year: 2008
• Volume: 6
• Issue: 2
• Pages: 185-193

Dates

published

1 - 6 - 2008

online

26 - 3 - 2008

Contributors

author

Xin-Fa Deng

• School of Science, Nanchang University, Jiangxi, China, 330031

author

Ji-Zhou He

• School of Science, Nanchang University, Jiangxi, China, 330031

author

Xin-sheng Ma

• School of Science, Nanchang University, Jiangxi, China, 330031

author

Peng Jiang

• School of Science, Nanchang University, Jiangxi, China, 330031

author

Xiao-Xun Tang

• School of Science, Nanchang University, Jiangxi, China, 330031

References

• [1] J.E. Barnes, Nature 338, 123 (1989) http://dx.doi.org/10.1038/338123a0[Crossref]
• [2] A. Cavaliere, S. Colafrancesco, R. Scaramella, Astrophys. J. 380, 15 (1991) http://dx.doi.org/10.1086/170557[Crossref]
• [3] R. Rampazzo, J.W. Sulentic, Astron. Astrophys. 259, 43 (1992)
• [4] A. Diaferio, M.J. Geller, M. Ramella, Astron. J. 107, 868 (1994) http://dx.doi.org/10.1086/116900[Crossref]
• [5] H.J. Rood, M.F. Struble, Publ. Astron. Soc. Pac. 106, 413 (1994) http://dx.doi.org/10.1086/133393[Crossref]
• [6] J. Vennik, G.M. Richter, G. Longo, Astron. Nachr. 314, 393 (1993) http://dx.doi.org/10.1002/asna.2113140602[Crossref]
• [7] M. Ramella et al., Astron. J. 107, 1623, (1994) http://dx.doi.org/10.1086/116971[Crossref]
• [8] S. Sakai, R. Giovanelli, G. Wegner, Astron. J. 108, 33 (1994) http://dx.doi.org/10.1086/117042[Crossref]
• [9] A. Garcia, Astron. Astrophys. 297, 56 (1995)
• [10] E. Barton et al., Astron. J. 112, 871 (1996) http://dx.doi.org/10.1086/118060[Crossref]
• [11] F. Governato, P. Tozzi, A. Cavaliere, Astrophys. J. 458, 18 (1996) http://dx.doi.org/10.1086/176789[Crossref]
• [12] P. Hickson, Annu. Rev. Astron. Astr. 35, 357 (1997) http://dx.doi.org/10.1146/annurev.astro.35.1.357[Crossref]
• [13] P. Hickson, Astrophys. J. 255, 382 (1982) http://dx.doi.org/10.1086/159838[Crossref]
• [14] I. Prandoni, A. Iovino, H.T. MacGillivray, Astron. J. 107, 1235 (1994) http://dx.doi.org/10.1086/116936[Crossref]
• [15] S. Allam, D. Tucker, Astron. Nachr. 321, 101 (2000) http://dx.doi.org/10.1002/(SICI)1521-3994(200005)321:2<101::AID-ASNA101>3.0.CO;2-5[Crossref]
• [16] M.E. Merch’an, M.A.G. Maia, D.G. Lambas, Astrophys. J. 545, 26 (2000) http://dx.doi.org/10.1086/317772[Crossref]
• [17] P. Focardi, B. Kelm, Astron. Astrophys. 391, 35 (2002) http://dx.doi.org/10.1051/0004-6361:20020377[Crossref]
• [18] A. Iovino, Astron. J. 124, 2471 (2002) http://dx.doi.org/10.1086/343059[Crossref]
• [19] M.E. Merch’an, A. Zandivarez, Mon. Not. R. Astron. Soc. 335, 216 (2002) http://dx.doi.org/10.1046/j.1365-8711.2002.05623.x[Crossref]
• [20] A. Iovino et al., Astron. J. 125, 1660 (2003) http://dx.doi.org/10.1086/373999[Crossref]
• [21] V.R. Eke et al., Mon. Not. R. Astron. Soc. 348, 866 (2004) http://dx.doi.org/10.1111/j.1365-2966.2004.07408.x[Crossref]
• [22] M.E. Merch’an, A. Zandivarez, Astrophys. J. 630, 759 (2005) http://dx.doi.org/10.1086/427989[Crossref]
• [23] B.C Lee et al., Astron. J. 127, 1811 (2004) http://dx.doi.org/10.1086/382236[Crossref]
• [24] C. Stoughton et al., Astron. J. 123, 485 (2002) http://dx.doi.org/10.1086/324741[Crossref]
• [25] K. Abazajian et al., Astron. J. 128, 502 (2004) http://dx.doi.org/10.1086/421365[Crossref]
• [26] C. J. Miller et al., Astron. J. 130, 968 (2005) http://dx.doi.org/10.1086/431357[Crossref]
• [27] A.A. Berlind et al., Astrophys. J. Suppl. S 167, 1 (2006) http://dx.doi.org/10.1086/508170[Crossref]
• [28] J.K. Adelman-McCarthy et al., Astrophys. J. Suppl. S 172, 634 (2007) http://dx.doi.org/10.1086/518864[Crossref]
• [29] X.F. Deng et al., Astron. Astrophys. 474, 783 (2007) http://dx.doi.org/10.1051/0004-6361:20066407[Crossref]
• [30] M. Davis, G. Efstathiou, C.S. Frenk, S.D.M. White, Astrophys. J. 292, 371 (1985) http://dx.doi.org/10.1086/163168[Crossref]
• [31] M. A. Strauss et al., Astron. J. 124, 1810 (2002) http://dx.doi.org/10.1086/342343[Crossref]
• [32] J.K. Adelman-McCarthy et al., arXiv:0707.3413, Astrophys. J. Suppl. S (in press)
• [33] D.G. York et al., Astron. J. 120, 1579 (2000) http://dx.doi.org/10.1086/301513[Crossref]
• [34] J.E. Gunn et al., Astron. J. 116, 3040 (1998) http://dx.doi.org/10.1086/300645[Crossref]
• [35] M. Fukugita et al., Astron. J. 111, 1748 (1996) http://dx.doi.org/10.1086/117915[Crossref]
• [36] D.W. Hogg, et al., Astron. J. 122, 2129 (2001) http://dx.doi.org/10.1086/323103[Crossref]
• [37] J.A. Smith et al., Astron. J. 123, 2121 (2002) http://dx.doi.org/10.1086/339311[Crossref]
• [38] J.R. Pier et al., Astron. J. 125, 1559 (2003) http://dx.doi.org/10.1086/346138[Crossref]
• [39] C. Park et al., Astrophys. J. 633, 11 (2005) http://dx.doi.org/10.1086/452625[Crossref]
• [40] M.R. Blanton et al., Astron. J. 125, 2348 (2003) http://dx.doi.org/10.1086/342935[Crossref]
• [41] J. Einasto et al., Mon. Not. R. Astron. Soc. 206, 529 (1984)
• [42] K. Shimasaku et al., Astron. J. 122, 1238 (2001) http://dx.doi.org/10.1086/322094[Crossref]
• [43] C. Park, Y.Y. Choi, Astrophys. J. 635, L29 (2005) http://dx.doi.org/10.1086/499243[Crossref]
• [44] C. Yamauchi, T. Goto, Mon. Not. R. Astron. Soc., 359, 1557 (2005) http://dx.doi.org/10.1111/j.1365-2966.2005.08996.x[Crossref]
• [45] R.G. Abraham, S. van den Bergh, P.A. Nair, Astrophys. J. 588, 218 (2003) http://dx.doi.org/10.1086/373919[Crossref]
• [46] I. Strateva et al., Astron. J. 122, 1861 (2001) http://dx.doi.org/10.1086/323301[Crossref]
• [47] O. Nakamura et al., Astron. J. 125, 1682 (2003) http://dx.doi.org/10.1086/368135[Crossref]
• [48] M.R. Blanton et al., Astrophys. J. 594, 186 (2003) http://dx.doi.org/10.1086/375528[Crossref]
• [49] I.K. Baldry et al., Astrophys. J. 600, 681 (2004) http://dx.doi.org/10.1086/380092[Crossref]
• [50] M. Balogh et al., Astrophys. J. 615, L101 (2004) http://dx.doi.org/10.1086/426079[Crossref]
• [51] B. Kelm, P. Focardi, G. Sorrentino, Astron. Astrophys. 442, 117 (2005) http://dx.doi.org/10.1051/0004-6361:20041448[Crossref]
• [52] E.L. Turner, W.L.W. Sargent, Astrophys. J. 194, 587 (1974) http://dx.doi.org/10.1086/153277[Crossref]
• [53] J.C. Jackson, Mon. Not. R. Astron. Soc. 173, 41 (1975)
• [54] J.R.I. Gott, E.L. Turner, Astrophys. J. 213, 309 (1977) http://dx.doi.org/10.1086/155157[Crossref]
• [55] H.J. Rood, J.R. Dickel, Astrophys. J. 224, 724 (1978) http://dx.doi.org/10.1086/156422[Crossref]
• [56] A. Diaferio, et al., Astron. J. 105, 2035 (1993) http://dx.doi.org/10.1086/116581[Crossref]
• [57] M. Girardi, G. Giuricin, Astrophys. J. 540, 45 (2000) http://dx.doi.org/10.1086/309314[Crossref]
• [58] D.L. Tucker et al., Astrophys. J. Suppl. S 130, 237 (2000) http://dx.doi.org/10.1086/317348[Crossref]
• [59] G. Giuricin et al., Astrophys. J. 554, 857 (2001) http://dx.doi.org/10.1086/321390[Crossref]
• [60] W. Freudling, M.A. Prieto, Astron. Astrophys. 306, 39 (1996)
• [61] S.E. Zepf, Astrophys. J. 407, 448 (1993) http://dx.doi.org/10.1086/172528[Crossref]
• [62] X.F. Deng et al., Chin. J. Astron. Astrophys. 6, 411 (2006) http://dx.doi.org/10.1088/1009-9271/6/4/03[Crossref]

Identifiers

DOI

10.2478/s11534-008-0037-x