Abundances in the Galactic bulge

As reported above, OTU 1, OTU 2, and OTU 6 showed different abundances according to the farming condition, having higher abundances in both tomato genotypes grown under OF; OTU 5

Recent observations of the bulge display a gradient of the mean metallicity and of [Ƚ/Fe] with distance from galactic plane.. Bulge regions away from the plane are less

[r]

So reaction is fastest between most abundant, least charged pairs of nuclei, and increase in T is needed to make slower reactions significant.. H-burning is by far the

In each panel, we show two MDFs derived from the simulations: one based upon the use of all star particles belonging to the bulge, after ap- plication of the kinematic

As compared to high metallicity disc H II regions, CNSFR show values of the O 23 and the N2 parameters whose distributions are shifted to lower and higher values, respectively,

Ia, and also partially due to mas yields. Therefore, both IMF and massive stellar yields are playing a role here. It is evident that a ‘by eye’ inspection of these panels would

We also plotted the total oxygen abundances calculated from the electron temperatures measured using the direct method, only for the long-slit data of knot B, and those estimated