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- Gustafsson, BengtUppsala universitet,Institutionen för fysik och astronomi (author)
The chemical composition of solar-type stars in comparison with that of the Sun
- Article/chapterEnglish2010
Publisher, publication year, extent ...
- 2010-02-05
- Springer Science and Business Media LLC,2010
- printrdacarrier
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- LIBRIS-ID:oai:DiVA.org:uu-135410
- https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-135410URI
- https://doi.org/10.1007/s10509-009-0257-6DOI
Supplementary language notes
- Language:English
- Summary in:English
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Notes
- The question whether the solar chemical composition is typical for solar-type stars is analysed by comparing the Sun with different stellar samples, including a sample of stars with very similar parameters, solar twins. Although typical in terms of overall metallicity for stars of solar age and galactic orbit, the solar atmosphere is found to have abundances, as compared with solar twins, that indicate that its gas has once been affected by dust formation and dust separation. It is concluded that this may be related to the formation of the solar planetary system and its special properties.
Subject headings and genre
- NATURVETENSKAP Fysik hsv//swe
- NATURAL SCIENCES Physical Sciences hsv//eng
- Sun: abundances
- Stars: abundances
- Solar system: formation
- Planetary systems
- Physics
- Fysik
Added entries (persons, corporate bodies, meetings, titles ...)
- Melendez, Jorge (author)
- Asplund, Martin (author)
- Yong, David (author)
- Uppsala universitetInstitutionen för fysik och astronomi (creator_code:org_t)
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- In:Astrophysics and Space Science: Springer Science and Business Media LLC328:1-2, s. 185-1910004-640X1572-946X
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