activity
20102023
most citedThe orbits of subdwarf B + main-sequence binaries. I: The sdB+G0 system PG 1104+243

65 citations · 251 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2023★ 25 cited

MELCHIORS: The Mercator Library of High Resolution Stellar Spectroscopy

P. Royer, T. Merle, K. Dsilva +71

Over the past decades, libraries of stellar spectra have been used in a large variety of science cases, including as sources of reference spectra for a given object or a given spec…

astro-ph.SR2016★ 54 cited

The temperature and chronology of heavy-element synthesis in low-mass stars

Pieter Neyskens, Sophie Van Eck, Alain Jorissen +3

Roughly half of the heavy elements (atomic mass greater than that of iron) are believed to be synthesized in the late evolutionary stages of stars with masses between 0.8 and 8 sol…

astro-ph.SR2012★ 65 cited

The orbits of subdwarf B + main-sequence binaries. I: The sdB+G0 system PG 1104+243

J. Vos, R. H. Östensen, P. Degroote +18

The predicted orbital period histogram of an sdB population is bimodal with a peak at short (< 10 days) and long (> 250 days) periods. Observationally, there are many short-period…

astro-ph.SR2012★ 11 cited

Discovery of a TiO emission band in the infrared spectrum of the S star NP Aurigae

K. Smolders, T. Verhoelst, P. Neyskens +10

We report on the discovery of an infrared emission band in the Spitzer spectrum of the S-type AGB star NP Aurigae that is caused by TiO molecules in the circumstellar environment.…

astro-ph.SR2012★ 21 cited

Detection of gravity modes in the massive binary V380 Cyg from Kepler spacebased photometry and high-resolution spectroscopy

A. Tkachenko, C. Aerts, K. Pavlovski +17

We report the discovery of low-amplitude gravity-mode oscillations in the massive binary star V380 Cyg, from 180 d of Kepler custom-aperture space photometry and 5 months of high-r…

astro-ph.SR2012★ 39 cited

The Spitzer Spectroscopic Survey of S-type Stars

K. Smolders, P. Neyskens, J. A. D. L. Blommaert +28

S-type AGB stars are thought to be in the transitional phase between M-type and C-type AGB stars. Because of their peculiar chemical composition, one may expect a strong influence…