Laboratory and Astronomical Discovery of HydroMagnesium Isocyanide
Carlos Cabezas, Jose Cernicharo, Jose Luis Alonso, Marcelino Agundez,, Santiago Mata, Michel Guelin, Isabel Pe\~na

TL;DR
This paper reports the first laboratory and astronomical detection of hydromagnesium isocyanide (HMgNC) in the star IRC+10216, including precise laboratory measurements and identification of multiple rotational lines in space.
Contribution
It provides the first laboratory spectroscopic data and astronomical detection of HMgNC, confirming its presence in space and determining its abundance and rotational constants.
Findings
HMgNC detected in IRC+10216 with four rotational lines.
Laboratory and space rotational constants are consistent.
Column density of HMgNC estimated at (6±2)×10^11 cm^-2.
Abstract
We report on the detection of hydromagnesium isocyanide, HMgNC, in the laboratory and in the carbon rich evolved star IRC+10216. The J=1-0 and J=2-1 lines were observed in our microwave laboratory equipment in Valladolid with a spectral accuracy of 3\,KHz. The hyperfine structure produced by the Nitrogen atom was resolved for both transitions. The derived rotational constants from the laboratory data are =5481.4333(6)\,MHz, =2.90(8)\,KHz, and =-2.200(2)\,MHz. The predicted frequencies for the rotational transitions of HMgNC in the millimeter domain have an accuracy of 0.2-0.7\,MHz. Four rotational lines of this species, J=8-7, J=10-9, J=12-11 and J=13-12, have been detected towards IRC+10216. The differences between observed and calculated frequencies are 0.5\,MHz. The rotational constants derived from space frequencies are =5481.49(3)\,MHz and…
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