{ "id": "1806.10149", "version": "v1", "published": "2018-06-26T18:00:08.000Z", "updated": "2018-06-26T18:00:08.000Z", "title": "Lessons on the high-z Universe from local Laboratories: Extreme Environments in Blueberry Galaxies", "authors": [ "Yu Rong", "Huan Yang", "Hong-xin Zhang", "Thomas H. Puzia", "Igor V. Chilingarian", "Paul Eigenthaler", "Sangeeta Malhotra", "James E. Rhoads", "Junxian Wang", "Yasna Ordens-briceno", "Evelyn Johnston" ], "comment": "10 pages, 7 figures, 1 table; submitted to ApJ", "categories": [ "astro-ph.GA" ], "abstract": "A population of so-called \"blueberry\" dwarf galaxies with extremely blue colors, low-metallicities, and enormous ionization ratios, has recently been found by \\cite{Yang17}. As a pilot study of these blueberries, we investigate two new blueberry candidates, RGG\\,B and RGG\\,5, which have Hubble Space Telescope high-resolution images.~We find that RGG\\,B and RGG\\,5 are likely to be merging dwarf galaxies; RGG\\,B may have a close merging companion, and RGG\\,5 presents shell-like outskirts.~Yet the current evidence still cannot exclude the possibility that RGG~B is just disturbed by in-situ star formation through, e.g., outflows, rather than undergoing a merger.~All of the blueberries, including RGG\\,B and RGG\\,5, are located close to the theoretical maximum-starburst-line in the BPT diagram, have very high ionization parameters, and relatively low hardness ionizing radiation fields, exhibit nitrogen overabundances, and show extremely red mid-IR colors, and reside in the so-called \"ULIRGs/LINERs/Obscured AGN\" region.~Their specific star formation rates (sSFR) range among the most extreme and compare with those of extreme starbursts at high redshifts.~The blueberry galaxies may not harbor AGN, which may be due to their very early phases of the galaxy merging process.", "revisions": [ { "version": "v1", "updated": "2018-06-26T18:00:08.000Z" } ], "analyses": { "keywords": [ "blueberry galaxies", "extreme environments", "high-z universe", "local laboratories", "specific star formation rates" ], "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable" } } }