淡江大學機構典藏:Item 987654321/72734
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    Please use this identifier to cite or link to this item: https://tkuir.lib.tku.edu.tw/dspace/handle/987654321/72734


    Title: Dense gas in nearby galaxies : XI. Interstellar 12C/13C ratios in the central regions of M 82 and IC 342
    Authors: Chin, Y.N.;Henkel, C.;Mauersberger, R.;Whiteoak, J.B.
    Contributors: 淡江大學物理學系
    Keywords: : ISM: abundances – Galaxies: abundances – Radio lines: ISM – Radio lines: galaxies
    Date: 1998-01
    Issue Date: 2013-05-31 11:31:16 (UTC+8)
    Publisher: Les Ulis: EDP Sciences
    Abstract: (12) C / (13) C line intensity ratios have been derived from several carbon-bearing molecules to confine the range of carbon and oxygen isotope abundance ratios toward the nuclear regions of two infrared bright galaxies. The most stringent limits are obtained from CN mm-wave emission lines. Supplementary measurements toward the Galactic center region indicate that overall I(twCN)/I(thCN) line intensity ratios are giving lower limits to the corresponding ISOC abundance ratio. Toward M82 and IC342, we find ISOC > 40 and > 30. Therefore the smaller ISOC ratio of our own Galactic center region (25) may not be typical for central regions of galaxies which are more luminous in the infrared. The ISOC limits and data from various isotopic species of CO also infer ISOA abundance ratios of > 90 and > 125 for M82 and IC342, respectively. From the I(HCfoN) / I(HCfiN) line intensity ratio, ISON > 100 is derived for M82. Based on observations with the IRAM 30-m telescope, Pico Veleta, Spain and the Swedish-ESO Submillimetre Telescope (SEST) at the European Southern Observatory (ESO), La Silla, Chile
    Relation: Astronomy and Astrophysics 329, pp.443-450
    Appears in Collections:[Graduate Institute & Department of Physics] Journal Article

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