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SUMMARY:The Universal Rotation Curve of disk galaxies: probing dark matter
  and the local expansion rate
DTSTART;VALUE=DATE-TIME:20260916T143500Z
DTEND;VALUE=DATE-TIME:20260916T150000Z
DTSTAMP;VALUE=DATE-TIME:20261027T083837Z
UID:indico-contribution-31297@indico.ific.uv.es
DESCRIPTION:Speakers: Tiziano Schiavone (SISSA\, Trieste)\nThe Universal R
 otation Curve provides a powerful empirical framework to investigate the d
 istribution of luminous and dark matter in disk galaxies. By adopting norm
 alized radial and velocity coordinates\, we investigate the emergence of u
 niversal kinematic properties across galaxies with different masses and lu
 minosities. The resulting co-added rotation curves will be analyzed throug
 h different dark matter mass models to constrain the halo density profiles
 . Finally\, we discuss the use of the radial Tully–Fisher relation to ob
 tain an independent estimate of the Hubble constant in the local Universe.
  This work represents a first step toward a unified analysis of galaxy rot
 ation curves and their cosmological applications.\n\nhttps://indico.ific.u
 v.es/event/8160/contributions/31297/
LOCATION:
URL:https://indico.ific.uv.es/event/8160/contributions/31297/
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