Wobbling Galaxy Spin Axes in Dense Environments

Jaehyun Lee, Suk Kim, Hyunjin Jeong, Rory Smith, Hoseung Choi, Ho Seong Hwang, Seok Joo Joo, Hak Sub Kim, Youngdae Lee, Sukyoung Yi

Research output: Contribution to journalArticle

2 Citations (Scopus)

Abstract

The orientation of galaxy spin vectors within the large-scale structure has been considered an important test of our understanding of structure formation. We investigate the angular changes of galaxy spin vectors in clusters-denser environments than are normally focused upon-using hydrodynamic zoomed simulations of 17 clusters YZiCS and a set of complementary controlled simulations. The magnitude by which galaxies change their spin vector is found to be a function of their rotational support, with larger cumulative angular changes of spin vectors when they have initially lower V θ/σ. We find that both mergers and tidal perturbations can significantly swing spin vectors, with larger changes in spin vector for smaller pericenter distances. Strong tidal perturbations are also correlated with the changes in stellar mass and specific angular momentum of satellite galaxies. However, changes in spin vector can often result in a canceling out of previous changes. As a result, the integrated angular change is always much larger than the angular change measured at any instant. Also, overall, the majority of satellite galaxies do not undergo mergers or sufficiently strong tidal perturbation after infall into clusters, and thus they end up suffering little change to their spin vectors. Taken as a whole, these results suggest that any signatures of spin alignment from the large-scale structure will be preserved in the cluster environment for many gigayears.

Original languageEnglish
Article number69
JournalAstrophysical Journal
Volume864
Issue number1
DOIs
Publication statusPublished - 2018 Sep 1

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galaxies
perturbation
merger
angular momentum
stellar mass
simulation
hydrodynamics
alignment
signatures

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Lee, J., Kim, S., Jeong, H., Smith, R., Choi, H., Hwang, H. S., ... Yi, S. (2018). Wobbling Galaxy Spin Axes in Dense Environments. Astrophysical Journal, 864(1), [69]. https://doi.org/10.3847/1538-4357/aad54e
Lee, Jaehyun ; Kim, Suk ; Jeong, Hyunjin ; Smith, Rory ; Choi, Hoseung ; Hwang, Ho Seong ; Joo, Seok Joo ; Kim, Hak Sub ; Lee, Youngdae ; Yi, Sukyoung. / Wobbling Galaxy Spin Axes in Dense Environments. In: Astrophysical Journal. 2018 ; Vol. 864, No. 1.
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Lee, J, Kim, S, Jeong, H, Smith, R, Choi, H, Hwang, HS, Joo, SJ, Kim, HS, Lee, Y & Yi, S 2018, 'Wobbling Galaxy Spin Axes in Dense Environments', Astrophysical Journal, vol. 864, no. 1, 69. https://doi.org/10.3847/1538-4357/aad54e

Wobbling Galaxy Spin Axes in Dense Environments. / Lee, Jaehyun; Kim, Suk; Jeong, Hyunjin; Smith, Rory; Choi, Hoseung; Hwang, Ho Seong; Joo, Seok Joo; Kim, Hak Sub; Lee, Youngdae; Yi, Sukyoung.

In: Astrophysical Journal, Vol. 864, No. 1, 69, 01.09.2018.

Research output: Contribution to journalArticle

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Lee J, Kim S, Jeong H, Smith R, Choi H, Hwang HS et al. Wobbling Galaxy Spin Axes in Dense Environments. Astrophysical Journal. 2018 Sep 1;864(1). 69. https://doi.org/10.3847/1538-4357/aad54e