I was thinking about an eerie object, maybe likely to orbit A-type stars and earlier spectral types.
Since Neptune-sized carbon planets have been inferred around stellar degenerates, silicate jovians have been confirmed (HD 189733 b) and chthonian planets exist, may carbon-based hot jupiters around hot stars exist?
There is a lack of close in exoplanets around these stars and such objects would show very low densities (I think, if I'm wrong, correct me) and bloated radii.
Who know? Several low-mass close binaries with very hot primary could turn out planetary systems.
Moreover I point out Beta Pictoris bears a carbon-rich disk and more massive stars may retain much greater amounts.
Jupiter-sized planets may accrete, migrate and turn hot-carbojupiters.
They could be named "Carbonados", after the charming smoked diamonds.
Suggestions?