Physical scalings for our galaxy models.
|[M⊙]||[km s−1]||[pc]||[Myr]||[kpc]||[M⊙]||[LU TU−1]|
|A||M87||6.05 × 109||325||255||3.07||2.95||6.05 × 1011||320|
|B||M31||1.63 × 108||169||21.75||1.01||0.42||1.63 × 1010||733|
|C||MW||4.6 × 106||103||1.4||0.62||.092||4.6 × 108||2044|
Notes. Columns from left to right: (1) initial galaxy model series; (2) reference galaxy chosen for physical scalings of models in Col. (1); (3) observed SMBH mass in the reference galaxy; (4) observed velocity dispersion; (5) observed influence radius; (6, 7, 8) model units of time, length, and mass, respectively; (9) value of c (speed of light) used in our simulations in model units.
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