What is the definition of disc scalelength?

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Disc scalelength refers to a parameter that describes the distribution of stars within a disk galaxy, influencing its mass distribution based on a specific mass-to-light (M/L) ratio. While the term is commonly used in astrophysical research, it lacks a precise, universally accepted definition, leading to some ambiguity among researchers. The concept can vary in interpretation, particularly when discussing specific measurements like "2.5 scale lengths." Despite extensive searches, definitive explanations remain elusive, highlighting a gap in clarity for a term frequently encountered in academic literature. Overall, the discussion emphasizes the need for a clearer understanding of disc scalelength in the context of galaxy formation studies.
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Can anyone please give m the definition of disc scalelength?
 
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PCB said:
... disc scalelength

I assumed you typo'ed and there should be a gap between scale and length

there are a number of answers to that on google :)

come back if you have any specific question in what you read

Dave
 
thanks, I have googled the term and I have found numerous uses of the term, but no definition. If you can help I would very much appreciate it.
 
from ... http://arxiv.org/pdf/1004.1507.pdf -

Scale length of disc galaxies

comes -----

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

Dave
 
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

Dave
 
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.
 

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