Oxygen lines in solar granulation: II. Centre-to-limb variation, NLTE line formation, blends, and the solar oxygen abundance
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Pereira, Tiago; Asplund, Martin; Kiselman, D
Description
Context: There is a lively debate about the solar oxygen abundance and the role of 3D models in its recent downward revision. These models have been tested using high-resolution solar atlases of flux and disk-centre intensity. Further testing can be done
Collections | ANU Research Publications |
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Date published: | 2009 |
Type: | Journal article |
URI: | http://hdl.handle.net/1885/38006 |
Source: | Astronomy and Astrophysics |
DOI: | 10.1051/0004-6361/200912840 |
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File | Description | Size | Format | Image |
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01_Pereira_Oxygen_lines_in_solar_2009.pdf | 439.61 kB | Adobe PDF | ||
02_Pereira_Oxygen_lines_in_solar_2009.pdf | 809.52 kB | Adobe PDF |
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