{ "id": "2408.09252", "version": "v1", "published": "2024-08-17T16:51:01.000Z", "updated": "2024-08-17T16:51:01.000Z", "title": "Parabolic-like Trend in SiO Ratios throughout the Central Molecular Zone: Possible Signature of a Past Nuclear Activity in the Galactic Center", "authors": [ "Shunya Takekawa", "Tomoharu Oka", "Shiho Tsujimoto", "Hiroki Yokozuka", "Nanase Harada", "Miyuki Kaneko", "Rei Enokiya", "Yuhei Iwata" ], "comment": "9 pages, 4 figures, accepted for publication in the Astrophysical Journal Letters", "doi": "10.3847/2041-8213/ad6c51", "categories": [ "astro-ph.GA" ], "abstract": "We report the discovery of a characteristic trend in the intensity ratios of SiO emissions across the Central Molecular Zone (CMZ) of our Galaxy. Using the Nobeyama Radio Observatory 45-m telescope, we conducted large-scale, high-sensitivity imaging observations in molecular lines including SiO $J$=2$-$1 and CS $J$=2$-$1. By identifying SiO-emitting clouds and examining their intensity ratios relative to the other molecular lines, we unveiled a parabolic-like trend showing lower ratios near the Galactic nucleus, Sgr A$^*$, with gradual increases toward the edges of the CMZ. This pattern suggests a possible outburst of the nucleus within the last $\\sim 10^5$ yr, which may have propagated through the entire CMZ with strong shocks. Alternatively, the observed trend may also be attributed to the destruction of small dust grains by high-energy photons. Our results can potentially lead to a new perspective on the history of nuclear activity and its impact on the surrounding molecular environment.", "revisions": [ { "version": "v1", "updated": "2024-08-17T16:51:01.000Z" } ], "analyses": { "keywords": [ "central molecular zone", "past nuclear activity", "sio ratios throughout", "parabolic-like trend", "galactic center" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable" } } }