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First results on the multi-element Doppler imaging of the CP star HD 3980
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Astronomy and Space Physics.
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2008 (English)In: Contributions of the Astronomical Observatory Skalnate Pleso, ISSN 1335-1842, Vol. 38, no 2, 347-352 p.Article in journal (Refereed) Published
Abstract [en]

We present the first results of an ongoing analysis of the inhomogeneous elemental surface distribution in the lithium-rich magnetic Ap star HD 3980. To derive surface maps for Fe, Pr, Li, Gd and Cr the Doppler imaging inversion code INVERS12 was applied. For this work high resolution time-series observations obtained with the VLT Ultraviolet and Visual Echelle Spectrograph (UVES) were used.

Place, publisher, year, edition, pages
2008. Vol. 38, no 2, 347-352 p.
Keyword [en]
stars : chemically peculiar, stars : abundances, stars : individual : HD 3980
National Category
Physical Sciences
URN: urn:nbn:se:uu:diva-149676ISI: 000256514000038OAI: oai:DiVA.org:uu-149676DiVA: diva2:405818
Conference Information: CP/AP Workshop 2007 Vienna, AUSTRIA, SEP 10-14, 2007Available from: 2011-03-23 Created: 2011-03-22 Last updated: 2011-03-23Bibliographically approved

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