Good question. It's a value that I've seen.
This document says 0.8 - 1.2.
http://citeseerx.ist.psu.edu/viewdoc/download?doi=10.1.1.140.8948&rep=rep1&type=pdf
Search for "range" to find it.
This also has those values (0.82 - 1.2):
http://www.bumply.com/astro.html
document.formSums.txtInnerHab2.value =(0.82*Math.sqrt(parseFloat(lum)));
document.formSums.txtOuterHab2.value =(1.2*Math.sqrt(parseFloat(lum)));
Well, the first document you cited, when I search it for range, does indeed find 0.8 and 1.2
but those values are not about habitable zone ranges in that context. They refer to solar masses.
The second link does use a formula for calculating habitable zones,
in accordance with the 2300AD role-playing game rules.
In any event, habitable zones are tricky. They depend not only on the star, but also on the planet in question. I.e. the planet might have more or less greenhouse gases. Technically, if we could pump enough such gases into the atmosphere of Mars, it could be made habitable, yet it is outside the habitable zone (albeit not by a very wide margin).
At the end of the day, one has to make a rather arbitrary decision: What temperature range represents a habitable zone? The quote I posted earlier decides it is a 0 to 100 degrees celsius range (presumably because that is the range in which liquid water is possible). It entirely ignores the greenhouse effects of water vapour and other gases on planets in that range.
Apparently, the 2300AD rulebook thinks the margin should be narrower, and it might well be correct, at least when dealing with very Earth-similar conditions of life.
How about making the zone according to the liquid water range, but represented visually as a gradient; densest in the middle and thinning out towards either extreme?
EDIT: The first article seems to arrive at a habitable zone of about 0.8 to 1.7 AU. It doesn't provide the numbers directly, so I'm estimating them from the diagram (figure 2).