Signatures of intrinsic Li depletion and Li-Na anti-correlation in the metal-poor globular cluster NGC6397
arXiv:0906.2876 · doi:10.1051/0004-6361/200912524
Abstract
To alleviate the discrepancy between the prediction of the primordial lithium abundance in the universe and the abundances observed in Pop II dwarfs and subgiant stars, it has been suggested that the stars observable today have undergone photospheric depletion of Li. To constrain the nature of such depletion, we conduct a homogeneous analysis of a very large sample of stars in the metal-poor globular cluster NGC6397, covering well all evolutionary phases from below the main sequence turn-off to high up the red giant branch. Non-LTE Li abundances or abundance upper limits are obtained for all stars, and for a size-able sub-set of the targets also Na abundances are obtained. The sodium abundances are used to distinguish stars formed out of pristine material from stars formed out of material affected by pollution from a previous generation of more massive stars. The dwarfs, turn-off, and early subgiant stars form a thin abundance plateau, disrupted in the middle of the subgiant branch by the lithium dilution caused by the first dredge-up. A second steep abundance drop is seen at the red giant branch bump. The turn-off stars are more lithium-poor, by up to 0.1 dex, than subgiants that have not yet undergone dredge-up. In addition, hotter dwarfs are slightly more lithium-poor than cooler dwarfs, which may be a signature of the so-called Li dip in the cluster, commonly seen among PopI stars. A considerably large spread in Na abundance confirms that NGC6397 has suffered from intra-cluster pollution in its infancy and a limited number of Na-enhanced and Li-deficient stars strongly contribute to form a significant anti-correlation between the abundances of Na and Li. The inferred Li abundances are compared to predictions from stellar structure models including atomic diffusion and ad-hoc turbulence below the convection zone.
13 pages, 11 figures, accepted by A&A, minor language corrections and some references changed
References in corpus (21)
- A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Some Aspects of Measurement Error in Linear Regression of Astronomical Data
- Fast rotating massive stars and the origin of the abundance patterns in galactic globular clusters
- A Bitter Pill: The Primordial Lithium Problem Worsens
- Departures from LTE for neutral Li in late-type stars
- Thermohaline mixing: A physical mechanism governing the photospheric composition of low-mass giants
- A probable stellar solution to the cosmological lithium discrepancy
- Signatures of intrinsic Li depletion and Li-Na anti-correlation in the metal-poor globular cluster NGC6397
- On the self-enrichment scenario of galactic globular clusters: Constraints on the IMF
- First stars VII. Lithium in extremely metal poor dwarfs
- Atomic Diffusion and Mixing in Old Stars I. VLT/FLAMES-UVES Observations of Stars in NGC 6397
- Origin of the abundance patterns in Galactic globular clusters: constraints on dynamical and chemical properties of globular clusters
- 3D Hydrodynamical Simulations of Surface Convection in Red Giant Stars. Impact on spectral line formation and abundance analysis
- Lithium Abundances of Extremely Metal-Poor Turn-off Stars
- NLTE determination of the sodium abundance in a homogeneous sample of extremely metal-poor stars
- Lithium abundances of halo dwarfs based on excitation temperature. I. LTE
- Atomic diffusion and mixing in old stars II. Observations of stars in the globular cluster NGC 6397 with VLT/FLAMES-GIRAFFE
- Variations in the lithium abundances of turn off stars in the globular cluster 47 Tuc
- Absolute motions of globular clusters. II. [HST astrometry and VLT radial velocities in NGC6397]
- Deep inside low-mass stars
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- Signatures of intrinsic Li depletion and Li-Na anti-correlation in the metal-poor globular cluster NGC6397
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