期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 440, 期 2, 页码 1794-1809出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stu287
关键词
galaxies: abundances; galaxies: evolution
资金
- European Union [PIEF-GA-2010-274117]
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [1313472] Funding Source: National Science Foundation
- Science and Technology Facilities Council [ST/H00243X/1, ST/K004182/1, ST/L001381/1, ST/K004352/1] Funding Source: researchfish
- STFC [ST/K004352/1, ST/L001381/1, ST/K004182/1] Funding Source: UKRI
We present X-shooter observations of CASSOWARY 20 (CSWA 20), a star-forming (SFR similar to 6 M-circle dot yr(-1)) galaxy at z = 1.433, magnified by a factor of 11.5 by the gravitational lensing produced by a massive foreground galaxy at z = 0.741. We analysed the integrated physical properties of the H ii regions of CSWA 20 using temperature- and density-sensitive emission lines. We find the abundance of oxygen to be similar to 1/7 of solar, while carbon is similar to 50 times less abundant than in the Sun. The unusually low C/O ratio may be an indication of a particularly rapid time-scale of chemical enrichment. The wide wavelength coverage of X-shooter gives us access to five different methods for determining the metallicity of CSWA 20, three based on emission lines from H ii regions and two on absorption features formed in the atmospheres of massive stars. All five estimates are in agreement, within the factor of similar to 2 uncertainty of each method. The interstellar medium (ISM) of CSWA 20 only partially covers the star-forming region as viewed from our direction; in particular, absorption lines from neutrals and first ions are exceptionally weak. We find evidence for large-scale outflows of the ISM with speeds of up 750 km s(-1), similar to the values measured in other high-z galaxies sustaining much higher rates of star formation.
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