Analysis of NGC1948 F6:4 - a Star in a Young Association of the Large Magellanic Cloud

Details Analysis of NGC1948 F6:4 - a Star in a Young Association of the Large Magellanic Cloud Analysis of NGC1948 F6:4 - a Star in a Young Association of the Large Magellanic Cloud

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...272..116s&link_type=abstract

Astronomy and Astrophysics, Vol.272, NO. 1/MAYI, P. 116, 1993

Astronomy and Astrophysics

Astrophysics

19

Scientific paper

The analysis of a K star in the young association NGC 1948 shows that the metallicity is [Fe/H] ~ -0.4 dex. The C and N abundances and the ^12^C/^13^C ratio indicate that the star has undergone an extensive internal mixing. Oxygen is deficient relative to iron, but this deficiency is inside the limits found by Luck & Lambert (1992) for the LMC cepheids. The heavy elements, heavier than Zr, are overabundant relative to iron. This overabundance seems to be a characteristic of the Magellanic Clouds stars.

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