A family of models for spherical stellar systems

Scott Tremaine, Douglas O. Richstone, Yong Ik Byun, Alan Dressler, S. M. Faber, Carl Grillmair, John Kormendy, Tod R. Lauer

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Abstract

We describe a one-parameter family of models of stable spherical stellar systems in which the phase-space distribution function depends only on energy. The models have similar density profiles in their outer parts (p ∝ r-4) and central power-law density cusps, p ∝ r3-η, 0<η≤3. The family contains the Jaffe [MNRAS, 202, 995 (1983)] and Hernquist [ApJ, 356, 359 (1990)] models as special cases. We evaluate the surface brightness profile, the line-of-sight velocity dispersion profile, and the distribution function, and discuss analogs of King's core-fitting formula for determining mass-to-light ratio. We also generalize the models to a two-parameter family, in which the galaxy contains a central black hole; the second parameter is the mass of the black hole. Our models can be used to estimate the detectability of central black holes and the velocity-dispersion profiles of galaxies that contain central cusps, with or without a central black hole.

Original languageEnglish
Pages (from-to)634-644
Number of pages11
JournalAstronomical Journal
Volume107
Issue number2
Publication statusPublished - 1994 Feb 1

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All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Tremaine, S., Richstone, D. O., Byun, Y. I., Dressler, A., Faber, S. M., Grillmair, C., Kormendy, J., & Lauer, T. R. (1994). A family of models for spherical stellar systems. Astronomical Journal, 107(2), 634-644.