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Interpretation of the Core-Wing Anomaly of Balmer line profiles of cool Ap stars
Kochukhov, O
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Astronomy and Space Physics, Observational Astrophysics.
Bagnulo, S.
Barklem, Paul
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Astronomy and Space Physics, Observational Astrophysics.
2003 (English)
In:
IAUS 210, Modelling of stellar atmospheres, 2003, p. D17-
Conference paper, Published paper (Other scientific)
Place, publisher, year, edition, pages
2003. p. D17-
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URN:
urn:nbn:se:uu:diva-18272
OAI: oai:DiVA.org:uu-18272
DiVA, id:
diva2:46044
Available from:
2007-01-09
Created:
2007-01-09
Last updated:
2018-05-30
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Kochukhov, O
Barklem, Paul
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Barklem, Paul
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