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20152026
most citedCannibals in the thick disk: the young rich stars as evolved blue stragglers

96 citations · 821 across the 29 of their papers we have counts for

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astro-ph.SR2015★ 59 cited

Detailed homogeneous abundance studies of 14 Galactic s-process enriched post-AGB stars: In search of lead (Pb)

Kenneth De Smedt, Hans Van Winckel, Devika Kamath +4

This paper is part of a larger project in which we systematically study the chemical abundances of Galactic and extragalactic post-asymptotic giant branch (post-AGB) stars. Lead (P…

astro-ph.SR2015★ 83 cited

The WISE View of RV Tauri Stars

I. Gezer, H. Van Winckel, Z. Bozkurt +4

We present a detailed study based on infrared photometry of all Galactic RV Tauri stars from the General Catalogue of Variable Stars (GCVS). RV Tauri stars are the brightest among…

astro-ph.SR2015★ 2 cited

The role of binarity in Wolf-Rayet central stars of planetary nebulae

Brent Miszalski, Rajeev Manick, Vanessa McBride

Over a hundred planetary nebulae (PNe) are known to have H-deficient central stars that mimic the spectroscopic appearance of massive Wolf-Rayet stars. The formation of these low-m…

astro-ph.SR2015

Post-common-envelope Wolf-Rayet central stars of planetary nebulae

Brent Miszalski, Rajeev Manick, Vanessa McBride

Nearly 50 post-common-envelope (post-CE) close binary central stars of planetary nebulae (CSPNe) are now known. Most contain either main sequence or white dwarf (WD) companions tha…

astro-ph.SR2015★ 46 cited

Kepler's first view of O-star variability: K2 data of five O stars in Campaign 0 as a proof-of-concept for O-star asteroseismology

B. Buysschaert, C. Aerts, S. Bloemen +9

We present high-precision photometric light curves of five O-type stars observed with the refurbished {\it Kepler\/} satellite during its Campaign 0. For one of the stars, we also…

astro-ph.SR2015★ 54 cited

A radial velocity survey for post-common-envelope Wolf-Rayet central stars of planetary nebulae: First results and discovery of the close binary nucleus of NGC 5189

Rajeev Manick, Brent Miszalski, Vanessa McBride

The formation of Wolf-Rayet central stars of planetary nebulae ([WR] CSPNe) whose spectroscopic appearance mimics massive WR stars remains poorly understood. Least understood is th…