# 2007A&A...470..179P

 other querymodes : Identifierquery Coordinatequery Criteriaquery Referencequery Basicquery Scriptsubmission TAP Outputoptions Help

 Query : 2007A&A...470..179P

2007A&A...470..179P - Astronomy and Astrophysics, volume 470, 179-190 (2007/7-4)

Light nuclei in galactic globular clusters: constraints on the self-enrichment scenario from nucleosynthesis.

PRANTZOS N., CHARBONNEL C. and ILIADIS C.

Abstract (from CDS):

Hydrogen-burning is the root cause of the star-to-star abundance variations of light nuclei in Galactic globular clusters (GC). In the present work we constrain the physical conditions that gave rise to the observed abundance patterns of Li, C, N, O, Na, Mg, Al, as well as Mg isotopes in the typical case of NGC 6752. We perform nucleosynthesis calculations at constant temperature, adopting realistic initial abundances for the proto-cluster gas. We use a detailed nuclear reaction network and state-of-the-art nuclear reaction rates. Although simplistic, our analysis provides original results and new constraints on the self-enrichment scenario for GCs. Our parametric calculations allow us to determine a narrow range of temperature where the observed extreme abundances of all light elements and isotopes in NGC 6752 are nicely reproduced simultaneously. This agreement is obtained after mixing of the H-processed material with ∼30% of unprocessed gas. We show that the observed C-N, O-Na, Mg-Al, Li-Na and F-Na anticorrelations as well as the behaviour of the Mg isotopes can be recovered by assuming mixing with various dilution factors. Li production by the stars that build up the other abundance anomalies is not mandatory in the case of NGC 6752. Observations of O, Na, Mg and Al constrain the temperature range for H-burning; such temperatures are encountered in the two main candidate polluters'' proposed for GCs, namely massive AGBs and the most massive main-sequence stars. Furthermore, observations require dilution of H-burning processed material with pristine one. They provide no clue, however, as to the nature of the unprocessed material required for mixing. The complementary observations of the fragile Li and F clearly point to ISM origin for the mixed material.

Journal keyword(s): stars: abundances - galaxies: abundances - globular clusters: general - globular clusters: individual: NGC 6752

Full paper

 Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 NGC 5139 GlC 13 26 47.28 -47 28 46.1           ~ 3315 0
2 M 4 GlC 16 23 35.22 -26 31 32.7           ~ 1793 0
3 NGC 6397 GlC 17 40 42.09 -53 40 27.6     5.17     ~ 1918 0
4 NGC 6752 GlC 19 10 52.11 -59 59 04.4           ~ 1934 0

To bookmark this query, right click on this link: simbad:objects in 2007A&A...470..179P and select 'bookmark this link' or equivalent in the popup menu

2023.04.01-19:17:28