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The standard way of plotting stars differently is to make multiple calls to the stars function, for example:

p.stars(where=[_.ccdm.isnull(), _.magnitude < 8])

# plot multiple star systems with the standard circle with a line through it symbol
p.stars(
  where=[_.ccdm.notnull(), _.magnitude < 8],
  style__marker__symbol="circle_line",
)

In the Tycho catalog (which is what the Big Sky catalog is based on), the CCDM identifies components of multiple star systems (so if the CCDM is not null, then it's a multiple star according to the Tycho catalog).

I remember seeing a cross reference for WDS and HIP/TYC, but it seems the WDS website is having some issues right now so I can't access it.

For …

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@enzodbspace
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Answer selected by steveberardi
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