Dancing in the dark: galactic properties trace spin swings along the cosmic web

@article{Dubois2014DancingIT,
  title={Dancing in the dark: galactic properties trace spin swings along the cosmic web},
  author={Y. Dubois and C. Pichon and C. Welker and D. L. Borgne and J. Devriendt and C. Laigle and S. Codis and D. Pogosyan and S. Arnouts and K. Benabed and E. Bertin and J. Blaizot and F. Bouchet and Jean-Franccois Cardoso and S. Colombi and V. D. Lapparent and V. Desjacques and R. Gavazzi and S. Kassin and T. Kimm and H. Mccracken and B. Milliard and S. Peirani and S. Prunet and S. Rouberol and J. Silk and A. Slyz and T. Sousbie and R. Teyssier and L. Tresse and M. Treyer and D. Vibert and M. Volonteri},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2014},
  volume={444},
  pages={1453-1468}
}
  • Y. Dubois, C. Pichon, +30 authors M. Volonteri
  • Published 2014
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • A large-scale hydrodynamical cosmological simulation, Horizon-AGN , is used to investigate the alignment between the spin of galaxies and the large-scale cosmic filaments above redshift one. The analysis of more than 150 000 galaxies with morphological diversity in a 100h −1 Mpc comoving box size shows that the spin of low-mass, rotationdominated, blue, star-forming galaxies is preferentially aligned with their neighbouring filaments. High-mass, dispersion-dominated, red, quiescent galaxies… CONTINUE READING
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