English

New perspectives on galactic angular momentum, galaxy formation, and the Hubble Sequence

Astrophysics of Galaxies 2018-12-18 v1

Abstract

This paper provides a summary of our recent work on the scaling relations between the specific angular momentum j_* and mass M_* of the stellar parts of normal galaxies of different bulge fraction beta_*. We find that the observations are consistent with a simple model based on a linear superposition of disks and bulges that follow separate scaling relations of the form j_*d ~ M_*d^alpha and j_*b ~ M_*b^alpha with alpha = 0.67 +/- 0.07 but offset from each other by a factor of 8 +/- 2 over the mass range 8.9 <= log (M_*/M_Sun) <= 11.8. This model correctly predicts that galaxies follow a curved 2D surface in the 3D space of log j_*, log M_*, and beta_*.

Keywords

Cite

@article{arxiv.1812.06144,
  title  = {New perspectives on galactic angular momentum, galaxy formation, and the Hubble Sequence},
  author = {S. Michael Fall and Aaron J. Romanowsky},
  journal= {arXiv preprint arXiv:1812.06144},
  year   = {2018}
}

Comments

4 pages, 3 figures; in proceedings of Focus Meeting 6 (Galactic Angular Momentum), IAU General Assembly XXX; see complete proceedings at https://www.dropbox.com/s/07ay9ag2xelt1xs/fm6.pdf?dl=0

R2 v1 2026-06-23T06:43:05.057Z