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Line Identification of Schneider’s Star (BD+24°3675) Around H β

Published online by Cambridge University Press:  12 April 2016

Reinhold Kroll
Reinhold Kroll*
Affiliation:
Institut für Astronomie und Astrophysik, Am Hubland, D-8700 Würzburg

Abstract

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The line spectrum of BD +24°3675 is investigated from 4730 to 4990 Å. I discuss the presence of individual elements, including Rare Earths. The equivalent widths of all strong lines are given. Estimates of T eff and logg indicate that the star might be evolved with a low surface gravity. Indications for spectral line variability have been found.

Information

Type
I. General Properties of CP Stars
Information
International Astronomical Union Colloquium , Volume 138: Peculiar versus Normal Phenomena in A-Type and Related Stars , 1993 , pp. 178 - 181
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

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