Laboratory and astronomical discovery of magnesium dicarbide, MgC
arXiv:2210.17348 · doi:10.3847/2041-8213/aca144
Abstract
We report the detection of magnesium dicarbide, MgC, in the laboratory at centimeter wavelengths and assign MgC, MgC, and MgC to 14 unidentified lines in the radio spectrum of the circumstellar envelope of the evolved carbon star IRC+10216. The structure of MgC is found to be T-shaped with a highly ionic bond between the metal atom and the C unit, analogous to other dicarbides containing electropositive elements. A two-temperature excitation model of the MgC emission lines observed in IRC+10216 yields a very low rotational temperature of K, a kinetic temperature of K, and a column density of cm. The abundance of MgC relative to the magnesium-carbon chains MgCCH, MgCH, and MgCH is and provides a new constraint on the sequential radiative association-dissociative recombination mechanisms implicated in the production of metal-bearing molecules in circumstellar environments.
arXiv comment15 pages, 5 figures
References in corpus (8)
- Laboratory and Astronomical Discovery of HydroMagnesium Isocyanide
- An Interferometric Spectral-line Survey of IRC+10216 in the 345 GHz Band
- Gas phase atomic metals in the circumstellar envelope of IRC+10216
- IRC +10 216 in 3-D: morphology of a TP-AGB star envelope
- The Abundance of SiC2 in Carbon Star Envelopes: Evidence that SiC2 is a gas-phase precursor of SiC dust
- Detection of the linear radical HC4N in IRC+10216
- Magnesium radicals MgCN and MgCH in IRC+10216
- A 1.3 cm line survey toward IRC +10216
Cited by in corpus (5)
- The magnesium paradigm in IRC+10216: Discovery of MgCH, MgCN, MgCH, and MgCN
- Discovery of two metallic cyanoacetylides in IRC+10216: HMgCCCN and NaCCCN
- Detection of the linear SiC and SiC radicals in IRC\,+10216
- Leveraging MMW-MMW Double Resonance Spectroscopy to Understand the Pure Rotational Spectrum of Glycidaldehyde and 17 of Its Vibrationally Excited States
- Development of a glow-discharge ion-trap instrument for measuring effective radiative-association rate coefficients