J/other/Nat/498.198       NGC6752 AGB and RGB Na abundances    (Campbell+, 2013)
The following files can be converted to FITS (extension .fit or fit.gz)
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/other/Nat/498.198

drwxr-xr-x 19 cats archive 4096 Jun 16 18:10 [Up] drwxr-xr-x 4 cats archive 205 May 26 2021 [TAR file] -rw-r--r-- 1 cats archive 473 Oct 19 2013 .message -r--r--r-- 1 cats archive 3931 Oct 19 2013 ReadMe -r--r--r-- 1 cats archive 2068 Aug 14 2013 tables1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/other/Nat/498.198 Na abundances in NGC6752 (Campbell+, 2013) ================================================================================ Sodium content as a predictor of the advanced evolution of globular cluster stars. Campbell S.W., D'Orazi V., Yong D., Constantino T.N., Lattanzio J.C., Stancliffe R.J., Angelou G.C., Wylie-de Boer E.C., Grundahl F. <Nature, 498, 198-200 (2013)> =2013Natur.498..198C ================================================================================ ADC_Keywords: Clusters, globular ; Stars, giant ; Abundances Keywords: Stars Abstract: The asymptotic giant branch (AGB) phase is the final stage of nuclear burning for low-mass stars. Although Milky Way globular clusters are now known to harbour (at least) two generations of stars, they still provide relatively homogeneous samples of stars that are used to constrain stellar evolution theory. It is predicted by stellar models that the majority of cluster stars with masses around the current turn-off mass (that is, the mass of the stars that are currently leaving the main sequence phase) will evolve through the AGB phase. Here we report that all of the second-generation stars in the globular cluster NGC 6752 - 70 per cent of the cluster population - fail to reach the AGB phase. Through spectroscopic abundance measurements, we found that every AGB star in our sample has a low sodium abundance, indicating that they are exclusively first-generation stars. This implies that many clusters cannot reliably be used for star counts to test stellar evolution timescales if the AGB population is included. We have no clear explanation for this observation. Description: We obtained high-resolution spectra (R 24000) for a sample of 20 AGB stars and 24 red giant branch stars in the Galactic globular cluster NGC 6752. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 19 10 52.11 -59 59 04.4 NGC6752 = GCl 108 ----------------------------------------------------------

© Université de Strasbourg/CNRS

    • Contact