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

Published online by Cambridge University Press:  12 April 2016

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

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 Teff and logg indicate that the star might be evolved with a low surface gravity. Indications for spectral line variability have been found.

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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