activity
20182021
most citedBarium & related stars and their white-dwarf companions II. Main-sequence and subgiant stars

78 citations · 137 across the 5 of their papers we have counts for

collaborators

11 papers

astro-ph.SR202113 cited

The binary central star of the bipolar pre-planetary nebula IRAS 08005-2356 (V510 Pup)

Rajeev Manick, Brent Miszalski, Devika Kamath +5

Current models predict that binary interactions are a major ingredient for the formation of bipolar planetary nebulae (PNe) and pre-planetary nebulae (PPNe). Despite years of radia…

astro-ph.SR2019

Two's company, three's a crowd: SALT reveals the likely triple nature of the nucleus of the extreme abundance discrepancy factor planetary nebula Sp 3

B. Miszalski, R. Manick, T. Rauch +3

The substantial number of binary central stars of planetary nebulae (CSPNe) now known (50) has revealed a strong connection between binarity and some morphological features i…

astro-ph.SR2019

GK Car and GZ Nor: Two low-luminous, depleted RV Tauri stars

I. Gezer, H. Van Winckel, R. Manick +1

We performed a photometric and spectroscopic analysis of two RV Tauri stars GK Car and GZ Nor. Both objects are surrounded by hot circumstellar dust. Their pulsation periods, deriv…

astro-ph.SR2019

The spectroscopic binaries RV Tauri and DF Cygni

Rajeev Manick, Devika Kamath, Hans Van Winckel +7

Aim: The focus of this paper is on two famous but still poorly understood RV Tauri stars: RV Tau and DF Cyg. We aim at confirming their suspected binary nature and deriving their o…

astro-ph.SR201913 cited

The post-common-envelope binary nucleus of the planetary nebula IC~4776: Neither an anomalously long orbital period nor a Wolf-Rayet binary

B. Miszalski, R. Manick, H. Van Winckel +1

The orbital period distribution of close binary stars consisting of a white dwarf and a main-sequence star (WDMS) is a powerful observational constraint on population synthesis mod…

astro-ph.SR201978 cited

Barium & related stars and their white-dwarf companions II. Main-sequence and subgiant stars

A. Escorza, D. Karinkuzhi, A. Jorissen +12

Barium (Ba) dwarfs and CH subgiants are the less-evolved analogues of Ba and CH giants. They are F- to G-type main-sequence stars polluted with heavy elements by a binary companion…