English

Magnesium radicals MgC$_5$N and MgC$_6$H in IRC+10216

Astrophysics of Galaxies 2021-09-01 v1

Abstract

After the previous discovery of MgC3_3N and MgC4_4H in IRC+10216, a deeper Q-band (31.0-50.3 GHz) integration on this source had revealed two additional series of harmonically related doublets that we assigned on the basis of quantum mechanical calculations to the larger radicals MgC5_5N and MgC6_6H. The results presented here extend and confirm previous results on magnesium-bearing molecules in IRC\,+10216. We derived column densities of (4.7±\pm1.3)×\times1012^{12} for MgC5_5N and (2.0±\pm0.9)×\times1013^{13} for MgC6_6H, which imply that MgC5_5N/MgC3_3N=0.5 and MgC6_6H/MgC4_4H = 0.9. Therefore, MgC5_5N and MgC6_6H are present with column densities not so different from those of the immediately shorter analogs. The synthesis of these large magnesium cyanides and acetylides in IRC+10216 can be explained for their shorter counterparts by a two-step process initiated by the radiative association of Mg+^+ with large cyanopolyynes and polyynes, which are still quite abundant in this source, followed by the dissociative recombination of the ionic complexes.

Keywords

Cite

@article{arxiv.2108.01480,
  title  = {Magnesium radicals MgC$_5$N and MgC$_6$H in IRC+10216},
  author = {J. R. Pardo and C. Cabezas and J. P. Fonfría and M. Agúndez and B. Tercero and P. de Vicente and M. Guélin and J. Cernicharo},
  journal= {arXiv preprint arXiv:2108.01480},
  year   = {2021}
}

Comments

5 pages, 3 figures