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Spin Alignment in Analogues of The Local Sheet

Published online by Cambridge University Press:  12 October 2016

George J. Conidis*
Affiliation:
Department of Physics and Astronomy, York University, Toronto, Ontario, M3J 1P3, Canada email: gconidis@yorku.ca
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Abstract

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Tidal torque theory and simulations of large scale structure predict spin vectors of massive galaxies should be coplanar with sheets in the cosmic web. Recently demonstrated, the giants (Ks ⩽ -22.5 mag) in the Local Volume beyond the Local Sheet have spin vectors directed close to the plane of the Local Supercluster, supporting the predictions of Tidal Torque Theory. However, the giants in the Local Sheet encircling the Local Group display a distinctly different arrangement, suggesting that the mass asymmetry of the Local Group or its progenitor torqued them from their primordial spin directions. To investigate the origin of the spin alignment of giants locally, analogues of the Local Sheet were identified in the SDSS DR9. Similar to the Local Sheet, analogues have an interacting pair of disk galaxies isolated from the remaining sheet members. Modified sheets in which there is no interacting pair of disk galaxies were identified as a control sample.

Galaxies in face-on control sheets do not display axis ratios predominantly weighted toward low values, contrary to the expectation of tidal torque theory. For face-on and edge-on sheets, the distribution of axis ratios for galaxies in analogues is distinct from that in controls with a confidence of 97.6% & 96.9%, respectively. This corroborates the hypothesis that an interacting pair can affect spin directions of neighbouring galaxies.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Abadi, M. G., Navarro, J. F., Fardal, M., Babul, A., & Steinmetz, M., 2009, preprint (arXiv:0902.2477)Google Scholar
Aragón-Calvo, M. A., van de Weygaert, R., Jones, B. J. T., & van der Hulst, J. M. 2007, ApJ, 655, L5 Google Scholar
Bailin, J., Kawata, D., Gibson, B. K., Steinmetz, M., Navarro, J. F., Brook, C. B., Gill, S. P. D., Ibata, R. A., Knebe, A., Lewis, G. F., & Okamoto, T. 2005, ApJ, 627, 17B Google Scholar
Berentzen, I. & Shlosman, I., 2006, ApJ, 648, 807 CrossRefGoogle Scholar
Philip, B., Vincent, E., Carlos, S. F., Adrian, J., & Takashi, O., 2010, MNRAS, 404, 1137 Google Scholar
Cen, R., 2014, ApJ, 785, 15 Google Scholar
Cervantes-Sodi, B., Hernandez, X., & Park, C., 2010, MNRAS, 402, 1807 CrossRefGoogle Scholar
Codis, S., Pichon, C., Devriendt, J., et al. 2012, MNRAS, 427, 3320 Google Scholar
Croft, R. A. C., Di Matteo, T., Springel, V., & Hernquist, L., 2009, MNRAS, 400, 43 Google Scholar
Cuesta, A. J., Betancort-Rijo, J. E., Gottlöber, S., et al. 2008, MNRAS, 385, 867 CrossRefGoogle Scholar
Dubois, Y., Pichon, C., Welker, C., et al. 2014, MNRAS, 444, 1453 Google Scholar
Efstathiou, G. & Jones, B. J. T., 1979, MNRAS, 186, 133 Google Scholar
Faltenbacher, A., Gottlöber, S., Kerscher, M., & Müller, V. 2002, A&A, 395, 1 Google Scholar
Gustafsson, M., Fairbairn, M., & Sommer-Larsen, J., 2006, Phys. Rev. D, 74, 123522 Google Scholar
Hahn, O., Carollo, C. M., Porciani, C., & Dekel, A., 2007, MNRAS, 381, 41 Google Scholar
Hoyle, F., 1949, MNRAS, 109, 365 Google Scholar
Jones, B. J. T., van de Weygaert, R., & Arag on-Calvo, M. A., 2010, MNRAS, 408, 897 Google Scholar
Kazantzidis, S., Kravtsov, A. V., Zentner, A. R., Allgood, B., Nagai, D., & Moore, B., 2004, ApJ, 611, L73 Google Scholar
Lee, J. & Erdogdu, P., 2007, ApJ, 671, 1248 Google Scholar
McCall, M. L., 2014, MNRAS, 440, 405 Google Scholar
Paz, D. J., Stasyszyn, F., & Padilla, N. D., 2008, MNRAS, 389, 1127 Google Scholar
Peebles, P. J. E., 1969, ApJ, 155, 393 Google Scholar
Peebles, P. J. E. & Nusser, A., 2010, Nature, 465, 565 CrossRefGoogle Scholar
Peebles, P. J. E., Phelps, S. D., Shaya, E. J., & Tully, R. B., 2001, ApJ, 554, 104 Google Scholar
Porciani, C., Dekel, A., & Hoffman, Y., 2002, MNRAS, 332, 325 Google Scholar
Romano-Díaz, E., Shlosman, I., Heller, C., & Hoffman, Y., 2009, ApJ, 702, 1250 CrossRefGoogle Scholar
Sales, L. V., Navarro, J. F., Theuns, T., Schaye, J., White, S. D. M., Frenk, C. S., Crain, R. A., & Vecchia, C. D., 2012, 423, 1544Google Scholar
Schäfer, B. M., 2009, IJMPD, 18, 173 Google Scholar
Slosar, A. & White, M., 2009, JCAP, 6, 9 Google Scholar
Springel, V., White, S. D. M., & Hernquist, L., 2004, in Ryder, S., Pisano, D., Walker, M., Freeman, K., eds, Proc. IAU Symp. 220, Dark Matter in Galaxies. Astron. Soc. Pac., San Francisco, p. 421CrossRefGoogle Scholar
Tempel, E., Stoica, R. S., & Saar, E., 2013, MNRAS, 428, 1827 Google Scholar
Tempel, E. & Libeskind, N. I., 2013, ApJ, 775, L42 Google Scholar
Trowland, H. E., Lewis, G. F., & Bland-Hawthorn, J., 2013, ApJ, 762, 72 Google Scholar
Trujillo, I., Carretero, C., & Patiri, S. G., 2006, ApJ, 640, L111 CrossRefGoogle Scholar
Tully, R. B., Shaya, E. J., Karachentsev, I. D., Courtois, H. M., Kocevski, D. D., Rizzi, L., & Peel, A., 2008, ApJ, 676, 184 Google Scholar
van den Bosch, F. C., Abel, T., Croft, R. A. C., Hernquist, L., & White, S. D. M., 2002, ApJ, 576, 21 Google Scholar
Varela, J., Betancort-Rijo, J., Trujillo, I., & Ricciardelli, E., 2012, ApJ, 744, 82 Google Scholar
Wang, H., Mo, H. J., Jing, Y. P., Yang, X., & Wang, Y., 2011, MNRAS, 413, 1973 Google Scholar
White, S. D. M., 1984, ApJ, 286, 38 CrossRefGoogle Scholar
Yoshida, N., Abel, T., Hernquist, L., & Sugiyama, N., 2003, ApJ, 592, 645 CrossRefGoogle Scholar
Zhang, Y., Yang, X., Faltenbacher, A., et al., 2009, ApJ, 706, 747 Google Scholar
Zhang, Y., Yang, X., Wang, H., et al. 2013, ApJ, 779, 160 CrossRefGoogle Scholar