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alpha-process Elements in the Galaxy: A Possible GAIA Contribution
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Department of Physics and Astronomy, Theoretical Astrophysics.
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Faculty of Science and Technology, Astronomical observatory. Department of Physics and Astronomy, Theoretical Astrophysics.
2002 (English)In: Astrophysics and Space Science, 2002, p. 143-150Conference paper, Published paper (Other scientific)
Abstract [en]

The sensitivity of stellar spectra to α/Fe abundance changes is investigated with the aim to be detected photometrically and employed for the scientific goals of the GAIA mission. A grid of plane parallel, line blanketed, flux constant, LTE model atm
Place, publisher, year, edition, pages
2002. p. 143-150
Keywords [en]
Stars, photometry
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-44134OAI: oai:DiVA.org:uu-44134DiVA, id: diva2:72039
Available from: 2006-12-20 Created: 2006-12-20

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http://www.arxiv.org/pdf/astro-ph/0201464

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Edvardsson, Bengt

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