Nuclear and nonnuclear abundance patterns in the manganese stars

Details Nuclear and nonnuclear abundance patterns in the manganese stars Nuclear and nonnuclear abundance patterns in the manganese stars

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196..521c&link_type=abstract

Astrophysical Journal, vol. 196, Mar. 1, 1975, pt. 1, p. 521-524.

Astronomy and Astrophysics

Astrophysics

13

A Stars, Abundance, Manganese, Metallic Stars, Nuclear Astrophysics, Nuclear Fusion, Gallium, Iron, Phosphorus, Silicon, Stellar Spectra, Yttrium

Scientific paper

The manganese stars show abundance anomalies that are in conflict with the predictions of nuclear astrophysics. The paper stresses the deviations from the odd-even effect that occur for phosphorus, gallium, and yttrium. The abundance anomalies (e.g., the Mn/Fe ratio) in the iron peak are less serious; within the uncertainties of the current determinations, they may be explained in terms of the same processes that predict the solar-system abundances.

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