Dense gas in nearby galaxies : XI. Interstellar 12C/13C ratios in the central regions of M 82 and IC 342

淡江大學機構典藏 > 理學院 > 物理學系暨研究所 > 期刊論文 > Item 987654321/72734

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题名:	Dense gas in nearby galaxies : XI. Interstellar 12C/13C ratios in the central regions of M 82 and IC 342
作者:	Chin, Y.N.;Henkel, C.;Mauersberger, R.;Whiteoak, J.B.
贡献者:	淡江大學物理學系
关键词:	: ISM: abundances – Galaxies: abundances – Radio lines: ISM – Radio lines: galaxies
日期:	1998-01
上传时间:	2013-05-31 11:31:16 (UTC+8)
出版者:	Les Ulis: EDP Sciences
摘要:	(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
關聯:	Astronomy and Astrophysics 329, pp.443-450
显示于类别:	[物理學系暨研究所] 期刊論文

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