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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 Statement
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 sciences |
| Research Field: | Galactic astronomy |
| Objective Division: | Expanding Knowledge |
| Objective Group: | Expanding knowledge |
| Objective Field: | Expanding knowledge in the physical sciences |
| UTAS Author: | Lovell, JEJ (Dr Jim Lovell) |
| ID Code: | 98496 |
| Year Published: | 2014 |
| Web of Science® Times Cited: | 10 |
| Deposited By: | Mathematics and Physics |
| Deposited On: | 2015-02-18 |
| Last Modified: | 2017-11-03 |
| Downloads: | 231 View Download Statistics |
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