Discovery of two metallic cyanoacetylides in IRC+10216: HMgCCCN and NaCCCN
arXiv:2304.01066 · doi:10.1051/0004-6361/202346462
Abstract
We report on the detection of a series of six lines in the ultra-deep Q-band integration toward IRC+10216 carried out with the Yebes 40m telescope, which are in harmonic relation with integer quantum numbers J from 12 to 18. After a detailed analysis of all possible carriers, guided by high-level quantum chemical calculations, we conclude that the lines belong to HMgCCCN, named hydromagnesium cyanoacetylide. The rotational temperature and column density derived for HMgCCCN are 17.1 +/- 2.8K and (3.0 +/- 0.6) e12 cm-2, respectively. The observed abundance ratio between MgCCCN and HMgCCCN is 3. In addition, we report the discovery in space, also toward IRC+10216, of sodium cyanoacetylide, NaCCCN, for which accurate laboratory data are available. For this species we derive a rotational temperature of 13.5 +/- 1.7K and a column density of (1.2 +/- 0.2) e11 cm-2.
Accepted in Astronomy & Astrophysics as Letter to the Editor on April 3rd, 2023
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Cited by in corpus (5)
- Carbon-Chain Chemistry in the Interstellar Medium
- The magnesium paradigm in IRC+10216: Discovery of MgCH, MgCN, MgCH, and MgCN
- Detection of the linear SiC and SiC radicals in IRC\,+10216
- Deep survey of millimeter RRLs towards the planetary nebulae IC 418 and NGC 7027
- Development of a glow-discharge ion-trap instrument for measuring effective radiative-association rate coefficients