The scale length determines how the stars are distributed throughout a disk, and can be used to derive its mass distribution,
assuming a specific M/L ratio. Ultimately, this mass distribution is the primary constraint for determining the formation scenariothere are others
Thanks, that is helpful, but I was looking for a detailed definition so I could understand what, for instance, 2.5 scale lengths meant in a particular situation.
from what I read in a couple of papers whilst doing that searching for you
is that you are not going to get a better definition. It is something that is a little vague and varies between researcherssorry
that's about the best I can do or find
Thanks very much, your efforts are much appreciated. I cannot help but feel that a term used as much as it is in many formal papers is not well defined, and/or that definition is not easy to find--in this information age.