other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
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):
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
To bookmark this query, right click on this link: simbad:1999MNRAS.308..551W and select 'bookmark this link' or equivalent in the popup menu