The Spectrum of the Manganese-Scandium Star φ Herculis

Details The Spectrum of the Manganese-Scandium Star φ Herculis The Spectrum of the Manganese-Scandium Star φ Herculis

Aug 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970ap%26ss...8..267a&link_type=abstract

Astrophysics and Space Science, Volume 8, Issue 2, pp.267-274

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

Among manganese stars, ϕ Herculis is of great interest because of
the unusual strength of the scandium lines. We present intensity
measurements for numerous lines of Cii, Mg i, Mg ii, Si ii, Ca ii, Sc
ii, Ti ii, Cr ii, Mn i, Mn ii, Fe i, Fe ii, Co ii, Sr ii, Yii, and Zr
ii.

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