{ "id": "1308.2041", "version": "v1", "published": "2013-08-09T06:46:15.000Z", "updated": "2013-08-09T06:46:15.000Z", "title": "Difference in the spatial distribution between H_2O and CO_2 ices in M82 found with AKARI", "authors": [ "Mitsuyoshi Yamagishi", "Hidehiro Kaneda", "Daisuke Ishihara", "Shinki Oyabu", "Takashi Onaka", "Takashi Shimonishi", "Toyoaki Suzuki", "Young Chol Minh" ], "comment": "11 pages, 3 figures, 1 table, accepted for publication in the ApJ Letters", "categories": [ "astro-ph.GA" ], "abstract": "With AKARI, we obtain the spatially-resolved near-infrared (2.5 - 5.0 um) spectra for the nearby starburst galaxy M82. These spectra clearly show the absorption features due to interstellar ices. Based on the spectra, we created the column density maps of H_2O and CO_2 ices. As a result, we find that the spatial distribution of H_2O ice is significantly different from that of CO_2 ice; H_2O ice is widely distributed, while CO_2 ice is concentrated near the galactic center. Our result for the first time reveals variations in CO_2/H_2O ice abundance ratio on a galactic scale, suggesting that the ice-forming interstellar environment changes within a galaxy. We discuss the cause of the spatial variations in the ice abundance ratio, utilizing spectral information on the hydrogen recombination Br{\\alpha} and Br{\\beta} lines and the polycyclic aromatic hydrocarbon 3.3 um emission appearing in the AKARI near-infrared spectra.", "revisions": [ { "version": "v1", "updated": "2013-08-09T06:46:15.000Z" } ], "analyses": { "keywords": [ "spatial distribution", "ice abundance ratio", "nearby starburst galaxy m82", "difference", "column density maps" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/773/2/L37", "journal": "The Astrophysical Journal", "year": 2013, "month": "Aug", "volume": 773, "number": 2 }, "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1247230, "adsabs": "2013ApJ...773L..37Y" } } }