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2015 | 13 | 1 |
Article title

Environmental dependence of stellar velocity dispersion in the Main galaxy sample of SDSS DR10

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EN
Abstracts
EN
The aim of this work is to examine the environmental
dependence of stellar velocity dispersion in local
galaxies. In studies that likely suffer from the radial selection
effect, one has a preference for the use of volumelimited
samples. Two volume-limited samples with different
redshift and luminosity ranges were constructed from
the Main galaxy data of the Sloan Digital Sky Survey Data
Release 10 (SDSS DR10). Considering some drawbacks of
volume-limited samples, the apparent magnitude-limited
Main galaxy sample was also applied. Statistical analyses
in these different galaxy samples can reach the same conclusion:
galaxies with large stellar velocity dispersions exist
preferentially in high density regimes, while galaxies
with small stellar velocity dispersions are located preferentially
in low density regions, which is inconsistent with
that obtained at intermediate redshifts.
Publisher

Journal
Year
Volume
13
Issue
1
Physical description
Dates
online
11 - 11 - 2014
received
7 - 6 - 2014
accepted
9 - 9 - 2014
Contributors
author
References
  • [1] C. P. Ahn, R. Alexandroff, C. Allende Prieto et al., Astrophys. J.Suppl. S., 203, 21 (2012)
  • [2] C. P. Ahn, R. Alexandroff, C. Allende Prieto et al., Astrophys. J.Suppl. S., 211, 17 (2014)
  • [3] A. J. Barth, L. C. Ho,W. L.W. Sargent, Astrophys. J., 566, L13 (2002)
  • [4] M. L. Balogh, D. Schade, S. L. Morris et al., Astrophys. J., 504, L75(1998)
  • [5] M. L. Balogh, I. K. Baldry, R. Nichol et al., Astrophys. J., 615, L101(2004)
  • [6] M. L. Balogh, V. Eke, C. Miller et al., Mon. Not. R. Astron. Soc.,348, 1355 (2004)
  • [7] M. Bernardi, A. Renzini, L. da Costa, Astrophys. J., 508, L143(1998)
  • [8] M. Bernardi, R. K. Sheth, J. Annis et al., Astron. J., 125, 1882(2003)
  • [9] M. Bernardi, F. Shankar, J. B. Hyde et al., Mon. Not. R. Astron.Soc., 404, 2087 (2010)
  • [10] M. R. Blanton, D. W. Hogg, N. A. Bahcall et al., Astrophys. J.,594,186 (2003)
  • [11] M. R. Blanton, D. Eisenstein, D. W. Hogg et al., Astrophys. J.,629,143 (2005)
  • [12] V. Botte, S. Ciroi, F. Di Mille et al., Mon. Not. R. Astron. Soc., 356,789 (2005)
  • [13] M. J. I. Brown, R. L. Webster, B. J. Boyle, Mon. Not. R. Astron.Soc., 317, 782 (2000)
  • [14] M. C. Cooper, J. A. Newman, A. L. Coil et al., Mon. Not. R. Astron.Soc., 376, 1445 (2007)
  • [15] O. Cucciati, A. Iovino, C.Marinoni et al., Astron. Astrophys., 458,39 (2006)
  • [16] X. F. Deng, J. Z.He, P. Jiang, Astrophys. J., 671, L101 (2007)
  • [17] X. F. Deng, J. Z. He, J. Song et al., PASP, 120, 487 (2008)
  • [18] X. F. Deng, J. Z. He, P. Wu, Astron. Astrophys., 484, 355 (2008)
  • [19] X. F. Deng, J. Z. He, X. Q. Wen, Mon. Not. R. Astron. Soc., 395, L90(2009)
  • [20] X. F. Deng, J. Z. He, X. Q. Wen, Astrophys. J., 693, L71 (2009)
  • [21] X. F. Deng, Astrophys. J., 721, 809 (2010)
  • [22] X. F. Deng, B. Yang, J. Z. He et al., Astrophys. J., 708, 101 (2010)
  • [23] X. F. Deng, X. Q. Wen, J. Y. Xu et al., Astrophys. J., 716, 599 (2010)
  • [24] X. F. Deng, Y. Xin, P. Jiang et al., AN, 331, 746 (2010)
  • [25] X. F. Deng, Y. Q. Chen, P. Jiang, Chin. J. Phys., 49, 1137 (2011)
  • [26] X. F. Deng, Y. Xin, C. H. Luo et al., Ap, 54, 355 (2011)
  • [27] X. F. Deng, Y. Q. Chen, P. Jiang, Mon. Not. R. Astron. Soc., 417,453 (2011)
  • [28] X. F. Deng, Astron. J., 143, 15 (2012)
  • [29] X. F. Deng, P. Wu, X. X. Qian et al., PASJ, 64, 93 (2012)
  • [30] X. F. Deng, J. Song, Y. Q. Chen et al., Astrophys. J., 753, 166 (2012)
  • [31] X. F. Deng, J. Song, Y. Q. Chen et al., AstL, 38, 213 (2012)
  • [32] X. F. Deng, C. H. Luo, Y. Xin et al., RMxAA, 49, 181 (2013)
  • [33] X. F. Deng, C. H. Luo, Y. Xin et al., Baltic Astronomy, 22, 133 (2013)
  • [34] X. F. Deng, AN, submitted (2014)
  • [35] X. F. Deng, RAA, 14, 553 (2014)
  • [36] A. Dressler, A. J. Oemler, W. J. Couch et al., Astrophys. J., 490,577 (1997)
  • [37] D. J. Eisenstein, J. Annis, J. E. Gunn et al., Astron. J., 122, 2267(2001)
  • [38] D. J. Eisenstein, D. H. Weinberg, E. Agol et al., Astron. J., 142, 72(2011)
  • [39] G. Fasano, B. M. Poggianti,W. J. Couch et al., Astrophys. J., 542,673 (2000)
  • [40] L. Ferrarese, D. Merritt, Astrophys. J., 539, L9 (2000)
  • [41] A. Gallazzi, S. Charlot, J. Brinchmann et al., Mon. Not. R. Astron.Soc., 370, 1106 (2006)
  • [42] K. Gebhardt, R. Bender, G. Bower et al., Astrophys. J., 539, L13(2000)
  • [43] P. L. Gómez, R. C. Nichol, C. J. Miller et al., Astrophys. J., 584,210 (2003)
  • [44] T. Goto, C. Yamauchi, Y. Fujita et al., Mon. Not. R. Astron. Soc.,346, 601 (2003)
  • [45] J. E. Greene, L. C. Ho, Astrophys. J., 641, 117 (2006)
  • [46] J. E. Greene, L. C. Ho, Astrophys. J., 641, L21 (2006)
  • [47] R. Grützbauch, C. J. Conselice, J. Varela et al., Mon. Not. R. Astron.Soc., 411, 929 (2011)
  • [48] R. Grützbauch, R. W. Chuter, C. J. Conselice, et al., Mon. Not. R.Astron. Soc., 412, 2361 (2011)
  • [49] N. Gruel, R. Guzmán, D. Cristóbal-Hornillos et al., Mon. Not. R.Astron. Soc., 420, 346 (2012)
  • [50] Y. Hashimoto, A. Oemler, J. H. Lin et al., Astrophys. J., 499, 589(1998)
  • [51] D. W. Hogg, M. R. Blanton, J. Brinchmann et al., Astrophys. J.,601, L29 (2004)
  • [52] J. Hu, Mon. Not. R. Astron. Soc., 386, 2242 (2008)
  • [53] G. Kauffmann, S. D. M. White, T. M. Heckman et al., Mon. Not. R.Astron. Soc., 353, 713 (2004)
  • [54] H. Kuntschner, R. J. Smith, M. Colless et al., Mon. Not. R. Astron.Soc., 337, 172 (2002)
  • [55] B. C. Lee, S. S. Allam, D. L. Tucker et al., Astron. J., 127, 1811(2004)
  • [56] I. Lewis, M. Balogh, R. De Propis et al., Mon. Not. R. Astron. Soc.,334, 673 (2002)
  • [57] C. Li, G. Kauffmann, Y. P. Jing et al., Mon. Not. R. Astron. Soc.,368, 21 (2006)
  • [58] J.Martinez-Manso, R.Guzmán, G. Barro et al., Astrophys. J., 738,22 (2011)
  • [59] A. Matković, R. Guzmán, Mon. Not. R. Astron. Soc., 362, 289(2005)
  • [60] C. Mendes de Oliveira, P. Coelho, J. J. González et al., Astrophys.J., 130, 55 (2005)
  • [61] P. Norberg, C. M. Baugh, E. Hawkins et al., Mon. Not. R. Astron.Soc., 328, 64 (2001)
  • [62] C. Park, Y. Y. Choi, M. S. Vogeley et al., Astrophys. J., 633, 11(2005)
  • [63] S. G. Patel, B. P. Holden, D. D. Kelson et al., Astrophys. J., 705,L67 (2009)
  • [64] M. Postman, M. J. Geller, Astrophys. J., 281, 95 (1984)
  • [65] R. Proctor, D. Forbes, G. Hau et al., Mon. Not. R. Astron. Soc.,349, 1381 (2004)
  • [66] K. Rakos, J. Schombert, A. Odell, Astrophys. J., 658, 929 (2007)
  • [67] D. S. Reed, F. Governato, T. Quinn et al., Mon. Not. R. Astron.Soc., 378, 777 (2007)
  • [68] P. Sánchez-Blázquez, J. Gorgas, N. Cardiel et al., Astron. Astrophys.,457, 809 (2006)
  • [69] O. K. Siĺchenko, Astrophys. J., 641, 229 (2006)
  • [70] R. J. Smith, J. R. Lucey, J. Price et al., Mon. Not. R. Astron. Soc.,419, 3167 (2012)
  • [71] C. Stoughton, R. H. Lupton, M. Bernardi, et al., Astron. J., 123,485 (2002)
  • [72] M. A. Strauss, D. H. Weinberg, R. H. Lupton, et al., Astron. J., 124,1810 (2002)
  • [73] M. Tanaka, T. Goto, S. Okamura et al., Astron. J., 128, 2677(2004)
  • [74] A. Terlevich, D. Forbes, Mon. Not. R. Astron. Soc., 330, 547(2002)
  • [75] D. Thomas, C. Maraston, R. Bender, C. Mendes de Oliveira, Astrophys.J., 621, 673 (2005)
  • [76] S. C. Trager, S. M. Faber, G. Worthey et al., Astron. J., 120, 165(2000)
  • [77] S. Tremaine, K. Gebhardt, R. Bender et al., Astrophys. J., 574,740 (2002)
  • [78] T. Treu, R. S. Ellis, J. Kneib et al., Astrophys. J., 591, 53 (2003)
  • [79] J. van de Sande, M. Kriek, M. Franx et al., Astrophys. J., 736, 9(2011)
  • [80] P. G. van Dokkum, M. Kriek, M. Franx, Nature, 460, 717 (2009)
  • [81] D. A. Wake, P. G. van Dokkum, M. Franx, Astrophys. J., 751, 44(2012)
  • [82] G. Wegner, N. A. Grogin, Astron. J., 136, 1 (2008)
  • [83] A. Zandivarez, H. J.Martínez, M. E. Merchán et al., Astrophys. J.,650, 137 (2006)
  • [84] I. Zehavi, M. R. Blanton, J. A. Frieman et al., Astrophys. J., 571,172 (2002)
Document Type
Publication order reference
Identifiers
YADDA identifier
bwmeta1.element.-psjd-doi-10_1515_phys-2015-0013
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