SIMBAD references

2016A&A...595A..16T - Astronomy and Astrophysics, volume 595A, 16-16 (2016/11-1)

CNO abundances and carbon isotope ratios in evolved stars of the open clusters NGC 2324, NGC 2477, and NGC 3960.

TAUTVAISIENE G., DRAZDAUSKAS A., BRAGAGLIA A., RANDICH S. and ZENOVIENE R.

Abstract (from CDS):

Aims. Our main aim is to determine carbon-to-nitrogen and carbon isotope ratios for evolved giants in the open clusters NGC 2324, NGC 2477, and NGC 3960, which have turn-off masses of about 2M, and to compare them with predictions of theoretical models.
Methods. High-resolution spectra were analysed using a differential synthetic spectrum method. Abundances of carbon were derived using the C2 Swan (0, 1) band heads at 5135 and 5635.5Å. The wavelength interval 7940-8130Å with strong CN features was analysed to determine nitrogen abundances and carbon isotope ratios. The oxygen abundances were determined from the [OI] line at 6300Å.
Results. The mean values of the CNO abundances are [C/Fe]=-0.35±0.06 (s.d.), [N/Fe]=0.28±0.05, and [O/Fe]=-0.02±0.10 in seven stars of NGC 2324; [C/Fe]=-0.26±0.02, [N/Fe]=0.39±0.04, and [O/Fe]=-0.11±0.06 in six stars of NGC 2477; and [C/Fe]=-0.39±0.04, [N/Fe]=0.32±0.05, and [O/Fe]=-0.19±0.06 in six stars of NGC 3960. The mean C/N ratio is equal to 0.92±0.12, 0.91±0.09, and 0.80±0.13, respectively. The mean 12C/13C ratio is equal to 21±1, 20±1, and 16±4, respectively. The 12C/13C and C/N ratios of stars in the investigated open clusters were compared with the ratios predicted by stellar evolution models.
Conclusions. The mean values of the 12C/13C and C/N ratios in NGC 2324 and NGC 2477 agree well with the first dredge-up and thermohaline-induced extra-mixing models, which are similar for intermediate turn-off mass stars. The 12C/13C ratios in the investigated clump stars of NGC 3960 span from 10 to 20. The mean carbon isotope and C/N ratios in NGC 3960 are close to predictions of the model in which the thermohaline- and rotation-induced (if rotation velocity at the zero-age main sequence was 30% of the critical velocity) extra-mixing act together.

Abstract Copyright: © ESO, 2016

Journal keyword(s): stars: abundances - stars: horizontal-branch - stars: evolution - open clusters and associations: individual: NGC 2324 - open clusters and associations: individual: NGC 2477 - open clusters and associations: individual: NGC 3960

CDS comments: Table 1 NGC 2477 13385 not identified.

Simbad objects: 36

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2016A&A...595A..16T and select 'bookmark this link' or equivalent in the popup menu


2019.12.12-12:18:44

© Université de Strasbourg/CNRS

    • Contact