A dimensionless quantity characterizing the → interstellar extinction,
defined by the total-to-selective extinction ratio:
RV = AV/E(B-V).
The typical value found for the reddening parameter in the Milky Way is
RV ~ 3.1, but it is known to vary from one
line of sight to another, from values as 2 to as large as 6.
Very large → dust grains would produce extinction
with RV → ∞.
See also: → reddening; → parameter.