In IRAS 06530-0213, HC3N and C4H emission is concentrated in an inner equatorial zone, and radiative-transfer modeling indicates HC3N's abundance, not just its excitation, peaks there.
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Interferometric molecular line observations toward the 21 {\mu}m protoplanetary nebula IRAS 06530-0213
In IRAS 06530-0213, HC3N and C4H emission is concentrated in an inner equatorial zone, and radiative-transfer modeling indicates HC3N's abundance, not just its excitation, peaks there.