Detailed analysis of the high-velocity giant HD 6497

Details Detailed analysis of the high-velocity giant HD 6497 Detailed analysis of the high-velocity giant HD 6497

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....43..127c&link_type=abstract

Astronomy and Astrophysics, vol. 43, no. 1, Sept. 1975, p. 127-131.

Astronomy and Astrophysics

Astrophysics

6

Giant Stars, Star Distribution, Stellar Evolution, Stellar Spectra, Abundance, Doppler Effect, Line Spectra, Mathematical Models, Stellar Gravitation, Stellar Temperature, Velocity Distribution

Scientific paper

This new detailed analysis of the high-velocity giant HD 6497 (K 2 III) shows the importance of using really weak lines in abundance determinations. The present analysis has been performed from curves of growth enriched in weak-lines. HD 6497 is found normal in iron-content in contrast of some previous determinations. This finding raises questions regarding the star's membership in the Arcturus moving group.

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