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19992014
most citedUsing Cepheids to determine the galactic abundance gradient I. The solar neighbourhood

173 citations · 523 across the 7 of their papers we have counts for

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astro-ph2002★ 135 cited

Using Cepheids to determine the galactic abundance gradient. III.First results for the outer disc

S. M. Andrievsky, V. V. Kovtyukh, R. E. Luck +3

As a continuation of our previous work, which concerned the radial abundance distribution in the galactic disc over the distances 4-10 kpc this paper presents the first results on…

astro-ph2001★ 173 cited

Using Cepheids to determine the galactic abundance gradient I. The solar neighbourhood

S. M. Andrievsky, V. V. Kovtyukh, R. E. Luck +7

A number of studies of abundance gradients in the galactic disk have been performed in recent years. The results obtained are rather disparate: from no detectable gradient to a rat…

astro-ph2001★ 145 cited

Using Cepheids to determine the galactic abundance gradient II. Towards the galactic center

S. M. Andrievsky, D. Bersier, V. V. Kovtyukh +4

Based on spectra obtained at the Anglo-Australian Observatory, we present a discussion of the metallicity of the galactic disc derived using Cepheids at galactocentric distances 4-…

astro-ph2000★ 12 cited

Helium contamination from the progenitor stars of planetary nebulae: The He/H radial gradient and the Delta Y/Delta Z enrichment ratio

W. J. Maciel

In this work, two aspects of the chemical evolution of 4He in the Galaxy are considered on the basis of a sample of disk planetary nebulae (PN). First, an application of correction…

astro-ph1999

Metallicity distribution of bulge planetary nebulae and the [O/Fe] x [Fe/H] relation

W. J. Maciel

The O/H metallicity distribution of different samples of planetary nebulae in the bulge of the Milky Way and M31 are compared. O/H abundances are converted into [Fe/H] metallicity…