selden wrote:Did you use that name when searching?
Yes.
selden wrote:At any rate, there are quite a few papers listed by Simbad for both objects. Both seem to be high in metals.
I only found two when I searched CN Leo, and none when searching Wolf 359. For the two I found, both of them seemed to hint at discussing metallicity, but they either didn't reveal CN Leo's metallicity, or it's in a format that I don't understand (I'm not quite a professional astronomer).
chaos syndrome wrote:Sirius B is a carbon/oxygen white dwarf (i.e. mostly made of "metals"), no?
Indeed, and I figured this would affect metallicity. However I cannot seem to find any actual value, much like with CN Leo.
[/quote]As for the metallicity of the progenitor, that's rather harder to figure out... the fact that Sirius A likely got contaminated during the red giant stage also makes things tricky.[/quote]
I've a metallicity of 0.2788 for Sirius A. I found a metallicity of 190% for Sirius A from somewhere, and
if I did the math right.