activity
19982025
most citedThe Distribution of the Elements in the Galactic Disk III. A Reconsideration of Cepheids from l = 30 to 250 Degrees

230 citations · 2k across the 49 of their papers we have counts for

collaborators

49 papers

astro-ph.GA2025

Classical Cepheids in the Galactic thin disk I. Abundance gradients via non-local thermodynamic equilibrium spectral analysis

Antonino Nunnari, Valentina D'Orazi, Giuliana Fiorentino +23

Classical Cepheids (CCs) have long been considered excellent tracers of the chemical evolution of the Milky Way's young disk. We present a homogeneous, NLTE spectroscopic analysis…

astro-ph.SR2024

Lithium Cepheid V708 Car with an unusual chemical composition

V. V. Kovtyukh, S. M. Andrievsky, K. Werner +2

The purpose of this work is to spectroscopically analyse the classical Cepheid V708 Car. A preliminary check of the spectrum of V708 Car showed that this is a lithium-rich supergia…

astro-ph.GA2023★ 32 cited

Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk

R. da Silva, V. D'Orazi, M. Palla +25

Classical Cepheids (CCs) are solid distance indicators and tracers of young stellar populations. Our aim is to provide iron, oxygen, and sulfur abundances for the largest and most…

astro-ph.SR2023★ 6 cited

Effective temperatures of classical Cepheids from line-depth ratios in the H-band

V. Kovtyukh, B. Lemasle, N. Nardetto +6

The technique of line depth ratios (LDR) is one of the methods to determine the effective temperature of a star. They are crucial in the spectroscopic studies of variable stars lik…

astro-ph.SR2023★ 1 cited

An enigma of Przybylski's star: is there promethium on its surface?

Sergei M. Andrievsky, Sergey A. Korotin, Klaus Werner +1

We carried out a new attempt to check for the presence promethium lines in the spectrum of HD101065 (Przybylski's star). The neutron capture element promethium does not have stable…

astro-ph.SR2023★ 1 cited

Probing the Przybylski star for Deuterium

Sergei M. Andrievsky, Valery V. Kovtyukh

The Przybylski star spectrum has been studied in order to search for deuterium lines. Since this star is extremely enriched in the s-process elements, which are the product of inte…