arXiv Analytics

Sign in

arXiv:1407.1699 [astro-ph.GA]AbstractReferencesReviewsResources

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

Published 2014-07-07Version 1

We present new detections of cyanodiacetylene (HC$_{5}$N) toward hot molecular cores, observed with the Tidbinbilla 34 m radio telescope (DSS-34). In a sample of 79 hot molecular cores, HC$_{5}$N was detected towards 35. These results are counter to the expectation that long chain cyanopolyynes, such as HC$_{5}$N, are not typically found in hot molecular cores, unlike their shorter chain counterpart HC$_{3}$N. However it is consistent with recent models which suggest HC$_{5}$N may exist for a limited period during the evolution of hot molecular cores.

Comments: 13 pages, 7 figures. Accepted for publication in MNRAS, July 3 2014
Categories: astro-ph.GA
Related articles: Most relevant | Search more
arXiv:1007.4223 [astro-ph.GA] (Published 2010-07-23)
Spectral Energy Distributions of 6.7 GHz methanol masers
arXiv:1907.00564 [astro-ph.GA] (Published 2019-07-01)
ATLASGAL -- physical parameters of dust clumps associated with 6.7 GHz methanol masers
arXiv:1402.2682 [astro-ph.GA] (Published 2014-02-11)
SMA millimeter observations of Hot Molecular Cores