activity
20002026
most citedPresent-day cosmic abundances. A comprehensive study of nearby early B-type stars and implications for stellar and Galactic evolution and interstellar dust models

472 citations · 5.5k across the 131 of their papers we have counts for

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Showing 2014Show all

10 papers · 1 filter

astro-ph.SR2014★ 8 cited

A non-LTE spectral analysis of the 3He and 4He isotopes in the HgMn star kappa Cancri

Natalia L. Maza, Maria-Fernanda Nieva, Norbert Przybilla

We present a pilot study on non-local thermodynamic equilibrium (NLTE) line-formation computations for the isotopes 3He and 4He in the mercury-manganese star kappa Cancri. The impa…

astro-ph.SR2014★ 84 cited

Fundamental properties of nearby single early B-type stars

Maria-Fernanda Nieva, Norbert Przybilla

Fundamental parameters of a sample of 26 apparently slowly-rotating single early B-type stars in the solar neighbourhood are presented and compared to high-precision data from deta…

astro-ph.SR2014★ 35 cited

B fields in OB stars (BOB): on the detection of weak magnetic fields in the two early B-type stars beta CMa and epsilon CMa

L. Fossati, N. Castro, T. Morel +15

Within the context of the "B fields in OB stars (BOB)" collaboration, we used the HARPSpol spectropolarimeter to observe the early B-type stars beta CMa (HD44743; B1 II/III) and ep…

astro-ph.SR2014★ 16 cited

The B Fields in OB Stars (BOB) Survey

T. Morel, N. Castro, L. Fossati +29

The B fields in OB stars (BOB) survey is an ESO large programme collecting spectropolarimetric observations for a large number of early-type stars in order to study the occurrence…

astro-ph.GA2014★ 49 cited

Stellar Metallicity of the Extended Disk and Distance of the Spiral Galaxy NGC 3621

Rolf-Peter Kudritzki, Miguel A. Urbaneja, Fabio Bresolin +2

Low resolution ESO VLT/FORS spectra of blue supergiant stars are analyzed to determine stellar metallicities (based on elements such as Fe, Ti, Mg) in the extended disk of the spir…

astro-ph.SR2014★ 54 cited

A new method for an objective, -based spectroscopic analysis of early-type stars

Andreas Irrgang, Norbert Przybilla, Ulrich Heber +4

A precise quantitative spectral analysis - encompassing atmospheric parameter and chemical elemental abundance determination - is time consuming due to its iterative nature and the…