A spatially resolved ALMA study of the binary carbon star V Hya finds carbon-chain molecules concentrated in the inner few hundred au of its expanding disk, unlike the shell-like distributions seen in spherical carbon stars.
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Molecular Distributions and Abundances in the Binary-Shaped Outflow of V Hya
A spatially resolved ALMA study of the binary carbon star V Hya finds carbon-chain molecules concentrated in the inner few hundred au of its expanding disk, unlike the shell-like distributions seen in spherical carbon stars.