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The 3D non-LTE sola...
The 3D non-LTE solar nitrogen abundance from atomic lines
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- Amarsi, Anish (author)
- Uppsala universitet,Teoretisk astrofysik
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- Grevesse, N. (author)
- Univ Liege, Ctr Spatial Liege, Ave Pre Aily, B-4031 Angleur Liege, Belgium.;Univ Liege, Space Sci Technol & Astrophys Res STAR Inst, Allee 6 Aout,17,B5C, B-4000 Liege, Belgium.
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- Grumer, Jon (author)
- Uppsala universitet,Teoretisk astrofysik
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- Asplund, M. (author)
- Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2600, Australia.
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- Barklem, Paul (author)
- Uppsala universitet,Teoretisk astrofysik
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- Collet, R. (author)
- Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, Ny Munkegade 120, DK-8000 Aarhus C, Denmark.
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(creator_code:org_t)
- 2020-04-29
- 2020
- English.
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In: Astronomy and Astrophysics. - : EDP SCIENCES S A. - 0004-6361 .- 1432-0746. ; 636
- Related links:
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http://arxiv.org/pdf...
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https://urn.kb.se/re...
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https://doi.org/10.1...
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Abstract
Subject headings
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- Nitrogen is an important element in various fields of stellar and Galactic astronomy, and the solar nitrogen abundance is crucial as a yardstick for comparing different objects in the cosmos. In order to obtain a precise and accurate value for this abundance, we carried out NI line formation calculations in a 3D radiative-hydrodynamicSTAGGER model solar atmosphere in full 3D non-local thermodynamic equilibrium (non-LTE). We used a model atom that includes physically motivated descriptions for the inelastic collisions of NI with free electrons and with neutral hydrogen. We selected five NI lines of high excitation energy to study in detail, based on their strengths and on their being relatively free of blends. We found that these lines are slightly strengthened from non-LTE photon losses and from 3D granulation effects, resulting in negative abundance corrections of around - 0.01 dex and - 0.04 dex, respectively. Our advocated solar nitrogen abundance is log (N) = 7.77, with the systematic 1 sigma uncertainty estimated to be 0.05 dex. This result is consistent with earlier studies after correcting for differences in line selections and equivalent widths.
Subject headings
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- atomic processes
- radiative transfer
- line: formation
- Sun: abundances
- Sun: photosphere
- stars: abundances
Publication and Content Type
- ref (subject category)
- art (subject category)
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