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New detections of HC5N towards hot cores associated with 6.7 GHz methanol masers

Citation

Green, C-E and Green, JA and Burton, MG and Horiuchi, S and Tothill, NFH and Walsh, AJ and Purcell, CR and Lovell, JEJ and Millar, TJ, New detections of HC5N towards hot cores associated with 6.7 GHz methanol masers, Monthly Notices of the Royal Astronomical Society, 443, (3) pp. 2252-2263. ISSN 0035-8711 (2014) [Refereed Article]


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Copyright 2014 the authors

DOI: doi:10.1093/mnras/stu1349

Abstract

We present new detections of cyanodiacetylene (HC5N) towards hot molecular cores, observed with the Tidbinbilla 34 m radio telescope (DSS–34). In a sample of 79 hot molecular cores, HC5N was detected towards 35. These results are counter to the expectation that long chain cyanopolyynes, such as HC5N, are not typically found in hot molecular cores, unlike their shorter chain counterpart HC3N. However, it is consistent with recent models which suggest HC5N may exist for a limited period during the evolution of hot molecular cores.

Item Details

Item Type:Refereed Article
Keywords:astrochemistry, stars: formation, ISM: clouds, ISM: molecules
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Galactic Astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:Lovell, JEJ (Dr Jim Lovell)
ID Code:98496
Year Published:2014
Web of Science® Times Cited:3
Deposited By:Mathematics and Physics
Deposited On:2015-02-18
Last Modified:2017-11-03
Downloads:76 View Download Statistics

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