activity
20052022
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 · 2.2k across the 47 of their papers we have counts for

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11 papers · 1 filter

astro-ph2008★ 59 cited

HD 271791: An Extreme Supernova Runaway B Star Escaping from the Galaxy

Norbert Przybilla, Maria-Fernanda Nieva, Ulrich Heber +1

Hyper-velocity stars (HVSs) were first predicted by theory to be the result of the tidal disruption of a binary system by a super-massive black hole (SMBH) that accelerates one com…

astro-ph2008★ 224 cited

A cosmic abundance standard: chemical homogeneity of the solar neighbourhood and the ISM dust-phase composition

Norbert Przybilla, Maria-Fernanda Nieva, Keith Butler

A representative sample of unevolved early B-type stars in nearby OB associations and the field is analysed to unprecedented precision using NLTE techniques. The resulting chemical…

astro-ph2008★ 41 cited

HVS7: a chemically peculiar hyper-velocity star

N. Przybilla, M. F. Nieva, A. Tillich +3

Context: Hyper-velocity stars are suggested to originate from the dynamical interaction of binary stars with the supermassive black hole in the Galactic centre (GC), which accelera…

astro-ph2008★ 62 cited

LMC origin of the hyper-velocity star HE 0437-5439. Beyond the supermassive black hole paradigm

N. Przybilla, M. F. Nieva, U. Heber +4

Context: Hyper-velocity stars move so fast that only a supermassive black hole (SMBH) seems to be capable to accelerate them. Hence the Galactic centre (GC) is their only suggested…

astro-ph2007

Accurate Quantitative Spectroscopy of OB Stars: C and N abundances near the Main Sequence

M. F. Nieva, N. Przybilla

We present a state-of-the-art analysis technique able to simultaneously reproduce the entire H and He spectra of OB-type stars in the visual and the near-IR and to derive highly ac…

astro-ph2007★ 73 cited

Carbon abundances of early B-type stars in the solar vicinity. Non-LTE line-formation for C II/III/IV and self-consistent atmospheric parameters

M. F. Nieva, N. Przybilla

Precise determinations of the chemical composition in early B-type stars consitute fundamental observational constraints on stellar and galactochemical evolution. Carbon is one of…