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

collaborators

47 papers

astro-ph.SR2022★ 11 cited

The Gaia-ESO survey: A spectroscopic study of the young open cluster NGC 3293

T. Morel, A. Blazère, T. Semaan +24

We present a spectroscopic analysis of the GIRAFFE and UVES data collected by the Gaia-ESO survey for the young open cluster NGC 3293. Archive spectra from the same instruments obt…

astro-ph.SR2022★ 19 cited

The Gaia-ESO Survey: The analysis of the hot-star spectra

R. Blomme, S. Daflon, M. Gebran +44

The Gaia-ESO Survey (GES) is a large public spectroscopic survey that has collected, over a period of 6 years, spectra of ~ 10^5 stars. This survey provides not only the reduced sp…

astro-ph.SR2018★ 8 cited

Detection of magnetic fields in He-rich early B-type stars using HARPSpol

S. P. Järvinen, S. Hubrig, I. Ilyin +4

We focus on early-B type stars with helium overabundance, for which the presence of a magnetic field has not previously been reported. The measurements were carried out using high-…

astro-ph.SR2018★ 11 cited

NLTE spectroscopic analysis of the He anomaly in subluminous B-type stars

D. Schneider, A. Irrgang, U. Heber +2

Several B-type main-sequence stars show chemical peculiarities. A particularly striking class are the He stars, which exhibit a remarkable enrichment of He with respect to…

astro-ph.SR2017★ 10 cited

Magnetic field geometry and chemical abundance distribution of the He-strong star CPD -57 3509

S. Hubrig, N. Przybilla, H. Korhonen +9

The magnetic field of CPD -57 3509 was recently detected in the framework of the BOB (B fields in OB stars) collaboration. We acquired low-resolution spectropolarimetric observatio…

astro-ph.SR2017★ 17 cited

A comprehensive study of young B stars in NGC 2264: I. Space photometry and asteroseismology

K. Zwintz, E. Moravveji, P. I. Papics +9

Space photometric time series of the most massive members of the young open cluster NGC 2264 allow us to study their different sources of variability down to the millimagnitude lev…