activity
20012023
most citedUsing Cepheids to determine the galactic abundance gradient I. The solar neighbourhood

173 citations · 499 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2023

Unique distant classical Cepheid OGLE GD-CEP-1353 with anomalously high abundances of s- and r-process elements

V. V. Kovtyukh, S. M. Andrievsky, K. Werner +1

While looking for recently discovered distant Cepheids with an interesting chemical composition, we noticed one star (OGLE GD-CEP-1353) with extremely large equivalent widths of sp…

astro-ph.SR2014★ 88 cited

New insights on Ba over-abundance in open clusters. Evidence for the intermediate neutron-capture process at play?

T. Mishenina, M. Pignatari, G. Carraro +6

Recently an increasing number of studies were devoted to measure the abundances of neutron-capture elements heavier than iron in stars belonging to Galactic Open Clusters (OCs). OC…

astro-ph.GA2014★ 17 cited

The Origin of the Young Pulsar PSR J0826+2637 and Its Possible Former Companion HIP 13962

N. Tetzlaff, B. Dincel, R. Neuhaeuser +1

We aim to identify the birth place of the young pulsar PSR J0826+2637 in order to determine its kinematic age and give constraints on its radial and spatial (kick) velocity. Since…

astro-ph.SR2012★ 30 cited

Accurate luminosities from the oxygen 7771-4 A triplet and the fundamental parameters of F-G supergiants

V. V. Kovtyukh, N. Gorlova, S. I. Belik

The oxygen 7771-4 A triplet is a good indicator of luminosity in A-G supergiants. However, its strength also depends on other atmospheric parameters. In this study, we present the…

astro-ph.GA2011★ 22 cited

Galactic restrictions on iron production by various Types of supernovae

I. A. Acharova, Yu. N. Mishurov, V. V. Kovtyukh

We propose a statistical method for decomposition of contributions to iron production from various sources: supernovae Type II and the subpopulations of supernovae Type Ia -- promp…

astro-ph2003★ 24 cited

Line profile variations in classical Cepheids. Evidence for non-radial pulsations?

V. V. Kovtyukh, S. M. Andrievsky, R. E. Luck +1

We have investigated line profiles in a large sample of Cepheid spectra, and found four stars that show unusual (for Cepheids) line profile structure (bumps or/and asymmetries). Th…