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| ===== On the Detection of Hexapentaenediylidenesilylene ===== | ===== On the Detection of Hexapentaenediylidenesilylene ===== |
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| J. R. Pardo, J. P. Fonfría, M. Agúndez, B. Tercero, C. Cabezas, L. Velilla-Prieto, M. Guélin, P. de Vicente, and J. Cernicharo\\ | J. R. Pardo, J. P. Fonfría, M. Agúndez, B. Tercero, C. Cabezas, L. Velilla-Prieto, M. Guélin, P. de Vicente, and J. Cernicharo\\ |
| reported on the\\ | reported on the\\ |
| **[[https://doi.org/10.1051/0004-6361/202555902|Detection of SiC<sub>6</sub> in IRC +10216 through //Q//-band lines]]**\\ | **[[https://doi.org/10.1051/0004-6361/202555902|Detection of SiC<sub>6</sub> in IRC +10216 through //Q//-band lines]]**\\ |
| //Astron. Astrophys.// **700**, L6 (2025).\\ | //Astron. Astrophys.// **700**, L6 (2025).\\ |
| Hexapentaenediylidenesilylene, also known as silaheptahexaenediylidene, was detected in a line survey of CW Leonis in the 31.0 to 50.3 GHz region carried out with the 40 m Yebes telescope. 14 transitions with //J'// = 26 − 31 and 33 − 40 were covered with mostly good signal-to-noise ratio. | Hexapentaenediylidenesilylene, also known as silaheptahexaenediylidene, was detected in a line survey of CW Leonis in the 31.0 to 50.3 GHz region carried out with the 40 m Yebes telescope. 14 transitions with //J'// = 26 − 31 and 33 − 40 were covered with mostly good signal-to-noise ratio. Of these, 8 were not or only slightly blended and 2 were partly unblended. A rotational temperature of ~19 K was determined, in agreement with the more uncertain ~21 K determined for SiC<sub>4</sub>. The latter molecule is almost a factor of 10 more abundant than SiC<sub>6</sub>.\\ |
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| | Contributor(s): H. S. P. Müller; 08, 2025 |
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