Fundamental plane distances and peculiar velicities of 140 groups and clusters of galaxies at low redshifts: the Hubble diagram

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We used the fundamental plane (FP) of early-type galaxies (data from the Sloan Digital Sky Survey) to measure the relative distances and peculiar velocities of 140 groups and clusters of galaxies at low redshifts ( z<0.12 ). We have constructed the Hubble diagram between the distances of galaxy groups/clusters and their radial velocities in the CMB reference frame in the flat ΛCDM model ( Ωm=0.3 , H0=70 km · s –1 Mpc –1 ).

We found that the standard logarithmic scatter of groups and clusters of galaxies on the Hubble diagram (minus peculiar velocities) is ± 0.0173 ( N = 140), which corresponds to the deviation of the Hubble constant 70 ± 2.8 km · s –1 Mpc –1 . For a sample of galaxy systems ( N = 63) with X-ray luminosity in the interval 0.151÷4×1044 erg/s we got 70 ± 2.1 km · s –1 Mpc –1 . The standard deviations of peculiar velocities with quadratic allowance for errors are equal to null 714 ± 7 km/s and 600 ± 7 km/s, respectively.

Five large superclusters of galaxies from the SDSS region show an average peculiar velocity relative to the CMB reference frame +240 ± 250 km/s. We did not detect the outflow of galactic systems from the void (Giant Void, α≈13h , δ≈40° , z≈0.107 ) formed by groups and clusters of galaxies.

作者简介

F. Kopylova

Special Astrophysical Observatory

编辑信件的主要联系方式.
Email: flera@sao.ru
俄罗斯联邦, Nizhny Arkhdz

A. Kopylov

Special Astrophysical Observatory

Email: flera@sao.ru
俄罗斯联邦, Nizhny Arkhdz

参考

  1. S. A. Gregory and L. A. Thompson, 222, 784 (1978).
  2. M. Jõeveer, J. Einasto, and E. Tago, Monthly Not. Roy. Astron. Soc. 185, 357 (1978).
  3. R. P. Kirshner, A. Oemler, P. L. Schechter, and S. A. Shectman, 248, L57 (1981).
  4. V. de Lapparent, M. J. Geller, and J. P. Huchra, 302, L1 (1986).
  5. A. I. Kopylov, D. Y. Kuznetsov, T. S. Fetisova, and V. F. Shvar tsman, in Large Scale Structures of the Universe, Proc. of the 130th Symp. of the IAU, dedicated to the memory of M. A. Aaronson (1950–1987) held in Balatonfured, Hungary, June 15–20, 1987; edited by J. Audouze, M.-C. Pelletan, and A. Szalay. IAU Symp. № 130 (Dordrecht: Kluwer Academic Publishers, 1988), p.129.
  6. J. R. Bond, L. Kofman, and D. Pogosyan, Nature 380(6575), 603 (1996).
  7. M. Einasto, J. Einasto, E. Tago, V. Müller, and H. Andernach, Astron. J. 122, 2222 (2001).
  8. Ia. B. Zeldovich, J. Einasto, and S. F. Shandarin, Nature 300(5891), 407 (1982).
  9. D. J. Batuski and J. O. Burns, Astron. J. 90, 1413 (1985).
  10. R. B. Tully, 303, 25 (1986).
  11. K. Y. Stavrev, Astron. and Astrophys. Suppl. Ser. 144, 323 (2000).
  12. A. I. Kopylov and F. G. Kopylova, Astron. and Astrophys. 382, 389 (2002).
  13. J. Einasto, I. Suhhonenko, G. Hütsi, E. Saar, et al., Astron. and Astrophys. 534, id. A128 (2011).
  14. A. Dressler, D. Lynden-Bell, D. Burstein, R. L. Davies, S. M. Fa ber, R. Terlevich, and G. Wegner, 313, 42 (1987).
  15. S. Djorgovski and M. Davis, 313, 59 (1987).
  16. G. Wegner, M. Colless, G. Baggley, R. L. Davies, E. Bertschinger, D. Burstein, R. K. McMahan, Jr., and R. P. Saglia, Astrophys. J. Suppl. 106, 1 (1996).
  17. M. J. Hudson, R. J. Smith, J. R. Lucey, D. J. Schlegel, and R. L. Davies, 512, L79 (1999).
  18. L. N. da Costa, M. Bernardi, M. V. Alonso, G. Wegner, C. N. A. Willmer, P. S. Pellegrini, M. A. G. Maia, and S. Zaroubi, 537(2), L81 (2000).
  19. M. Batiste and D. J. Batuski, Monthly Not. Roy. Astron. Soc. 436, 3331 (2013).
  20. H. Aihara, C. Allende Prieto, D. An, S. F. Anderson, et al., Astrophys. J. Suppl. 193(2), id. 29 (2011).
  21. F. G. Kopylova and A. I. Kopylov, Astron. Letters 40, 595 (2014).
  22. F. G. Kopylova and A. I. Kopylov, Astrophys. Bull. 72(4), 363 (2017).
  23. F. G. Kopylova and A. I. Kopylov, Astron. Astrophys. Trans. 32(2), 105 (2021).
  24. F. G. Kopylova and A. I. Kopylov, Astron. Letters 33, 211 (2007).
  25. C. Saulder, S. Mieske, W. W. Zeilinger, and I. Chilingarian, Astron. and Astrophys. 557, id. A21 (2013).
  26. J. J. Mohr and G. Wegner, Astron. J. 114, 25 (1997).
  27. R. G. Carlberg, H. K. C. Yee, E. Ellingson, S. L. Morris, et al., 485(1), L13 (1997).
  28. F. G. Kopylova, Astrophys. Bull. 68, 253 (2013).
  29. M. A. Strauss, D. H. Weinberg, R. H. Lupton, V. K. Narayanan, et al., Astron. J. 124(3), 810 (2002).
  30. I. V. Chilingarian, A. Melchior, and I. Y. Zolotukhin, Monthly Not. Roy. Astron. Soc. 405, 1409 (2010).
  31. I. Jorgensen, M. Franx, and P. Kjaergaard, Monthly Not. Roy. Astron. Soc. 280, 167 (1996).
  32. P. J. E. Peebles, Principles of Physical Cosmology (Princeton: Princeton University, 1993).
  33. M. J. Hudson, J. R. Lucey, R. J. Smith, and J. Steel, Monthly Not. Roy. Astron. Soc. 291, 488 (1997).
  34. M. Colless, R. P. Saglia, D. Burstein, R. L. Davies, R. K. McMa han, and G. Wegner, Monthly Not. Roy. Astron. Soc. 321(2), 277 (2001).
  35. R. A. Gibbons, A. S. Fruchter, and G. D. Bothun, Astron. J. 121, 649 (2001).
  36. R. B. Tully, H. M. Courtois, A. E. Dolphin, J. R. Fisher, et al., Astron. J. 146(4), id. 86 (2013).
  37. T. Mutabazi, 911(1), id. 16 (2021).
  38. A. I. Kopylov and F. G. Kopylova, Astrophys. Bull. 70, 243 (2015).
  39. E. J. Shaya, R. B. Tully, D. Pomaréde and A. Peel, 927(2), id. 168 (2022).
  40. F. G. Kopylova and A. I. Kopylov, Astrophys. Bull. 77, 347 (2022).
  41. F. G. Kopylova and A. I. Kopylov, Astrophys. Bull. 75, 424 (2020).
  42. F. G. Kopylova and A. I. Kopylov, Astrophys. Bull. 79, 1 (2024).
  43. A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, 876(1), id. 85 (2019).
  44. Planck Collaboration, et al., Astron. and Astrophys. 641, id. A6 (2020).
  45. N. A. Bahcall, M. Gramann, and R. Cen, 436, 23 (1994).

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