{ "id": "1804.11321", "version": "v1", "published": "2018-04-30T16:49:46.000Z", "updated": "2018-04-30T16:49:46.000Z", "title": "Complex organic molecules in the Galactic Centre: the N-bearing family", "authors": [ "S. Zeng", "I. Jiménez-Serra", "V. M. Rivilla", "S. Martín", "J. Martín-Pintado", "M. A. Requena-Torres", "J. Armijos-Abendaño", "D. Riquelme", "R. Aladro" ], "comment": "24 pages, 23 figures, 7 tables, accepted for publication in MNRAS", "categories": [ "astro-ph.GA" ], "abstract": "We present an unbiased spectral line survey toward the Galactic Centre (GC) quiescent giant molecular cloud (QGMC), G+0.693 using the GBT and IRAM 30$\\,$ telescopes. Our study highlights an extremely rich organic inventory of abundant amounts of nitrogen (N)-bearing species in a source without signatures of star formation. We report the detection of 17 N-bearing species in this source, of which 8 are complex organic molecules (COMs). A comparison of the derived abundances relative to H$_2$ is made across various galactic and extragalactic environments. We conclude that the unique chemistry in this source is likely to be dominated by low-velocity shocks with X-rays/cosmic rays also playing an important role in the chemistry. Like previous findings obtained for O-bearing molecules, our results for N-bearing species suggest a more efficient hydrogenation of these species on dust grains in G+0.693 than in hot cores in the Galactic disk, as a consequence of the low dust temperatures coupled with energetic processing by X-ray/cosmic ray radiation in the GC.", "revisions": [ { "version": "v1", "updated": "2018-04-30T16:49:46.000Z" } ], "analyses": { "keywords": [ "complex organic molecules", "galactic centre", "n-bearing family", "quiescent giant molecular cloud", "extremely rich organic inventory" ], "note": { "typesetting": "TeX", "pages": 24, "language": "en", "license": "arXiv", "status": "editable" } } }