SIMBAD references

1999MNRAS.308..551W - Mon. Not. R. Astron. Soc., 308, 551-556 (1999/September-2)

Collisional baryonic dark matter haloes.

WALKER M.A.

Abstract (from CDS):

If dark haloes are composed of dense gas clouds, as has recently been inferred, then collisions between clouds lead to galaxy evolution. Collisions introduce a core in an initially singular dark matter distribution, and can thus help to reconcile scale-free initial conditions - such as are found in simulations - with observed haloes, which have cores. A pseudo-Tully-Fisher relation, between halo circular speed and visible mass (not luminosity), emerges naturally from the model: Mvis∝V7/2.

Published data conform astonishingly well to this theoretical prediction. For our sample of galaxies, the mass-velocity relationship has much less scatter than the Tully-Fisher relation, and holds as well for dwarf galaxies (where diffuse gas makes a sizeable contribution to the total visible mass) as it does for giants. It seems very likely that this visible-mass/velocity relationship is the underlying physical basis for the Tully-Fisher relation, and this discovery in turn suggests that the dark matter is both baryonic and collisional.


Abstract Copyright: 1999, Royal Astronomical Society

Journal keyword(s): galaxies: evolution - galaxies: haloes - dark matter

Simbad objects: 17

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