Sulphur in the metal poor globular cluster NGC 6397

TL;DR

This study reports the first measurement of sulphur in a very metal-poor globular cluster, revealing its abundance pattern and suggesting sulphur's role in early cluster chemical evolution.

Contribution

It provides the first sulphur abundance measurement in a metal-poor globular cluster, extending knowledge to lower metallicities and comparing it with field stars.

Findings

Sulphur abundance in NGC 6397 is consistent with the Galactic halo plateau.

[S/Fe] ratio shows large scatter, possibly indicating multiple production channels.

Sulphur traces other alpha-elements and correlates with sodium, hinting at proton-capture processes.

Abstract

Sulphur (S) is a non-refractory alpha-element that is not locked into dust grains in the interstellar medium. Thus no correction to the measured, interstellar sulphur abundance is needed and it can be readily compared to the S content in stellar photospheres. Here we present the first measurement of sulphur in the metal poor globular cluster (GC) NGC 6397, as detected in a MIKE/Magellan high signal-to-noise, high-resolution spectrum of one red giant star. While abundance ratios of sulphur are available for a larger number of Galactic stars down to an [Fe/H] of ~ -3.5 dex, no measurements in globular clusters more metal poor than -1.5 dex have been reported so far. We find a NLTE, 3-D abundance ratio of [S/Fe] = +0.52 +/- 0.20 (stat.) +/- 0.08 (sys.), based on the S I, Multiplet 1 line at 9212.8A. This value is consistent with a Galactic halo plateau as typical of other alpha-elements in GCs and field stars, but we cannot rule out its membership with a second branch of increasing [S/Fe] with decreasing [Fe/H], claimed in the literature, which leads to a large scatter at metallicities around -2 dex. The [S/Mg] and [S/Ca] ratios in this star are compatible with a Solar value to within the (large) uncertainties. Despite the very large scatter in these ratios across Galactic stars between literature samples, this indicates that sulphur traces the chemical imprints of the other alpha-elements in metal poor GCs. Combined with its moderate sodium abundance ([S/Na]_NLTE=0.48), the [S/Fe] ratio in this GC extends a global, positive S-Na correlation that is not seen in field stars and might indicate that proton-capture reactions contributed to the production of sulphur in the (metal poor) early GC environments.