New detections of HC$_{5}$N toward hot cores associated with 6.7 GHz methanol masers
Claire-Elise Green, James A. Green, Michael G. Burton, Shinji, Horiuchi, Nicholas F. H. Tothill, Andrew J. Walsh, Cormac R. Purcell, James, E. J. Lovell, Thomas J. Millar

TL;DR
This study reports the detection of HC$_{5}$N in hot molecular cores, challenging previous assumptions and supporting models that predict its transient presence during core evolution.
Contribution
First detection of HC$_{5}$N in hot cores, providing evidence for its temporary existence during core evolution, contrary to prior expectations.
Findings
HC$_{5}$N detected in 35 out of 79 hot cores
Detection challenges previous assumptions about cyanopolyynes in hot cores
Supports models predicting transient HC$_{5}$N presence
Abstract
We present new detections of cyanodiacetylene (HCN) toward hot molecular cores, observed with the Tidbinbilla 34 m radio telescope (DSS-34). In a sample of 79 hot molecular cores, HCN was detected towards 35. These results are counter to the expectation that long chain cyanopolyynes, such as HCN, are not typically found in hot molecular cores, unlike their shorter chain counterpart HCN. However it is consistent with recent models which suggest HCN may exist for a limited period during the evolution of hot molecular cores.
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