activity
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

collaborators

7 papers

astro-ph.SR2014★ 57 cited

Oxygen abundance distribution in Galactic disc

S. A. Korotin, S. M. Andrievsky, R. E. Luck +3

We have performed a NLTE analysis of the infrared oxygen triplet for a large number of cepheid spectra obtained with the Hobby-Eberly telescope. These data were combined with our p…

astro-ph.GA2009★ 1 cited

Chemical evolution of the galactic bulge: single and double infall models

R. D. D. Costa, W. J. Maciel, A. V. Escudero

Recent work has produced a wealth of data concerning the chemical evolution of the galactic bulge, both for stars and nebulae. Present theoretical models generally adopt a limited…

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…