A catalogue of symbiotic stars

By Krzysztof Belczyński, J. Mikołajewska, U. Munari, R. Ivison, M. Friedjung. 2000

230 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH (2006, background): “Symbiotic stars (e.g. Belczyński et al. 2000) are one likely source of remaining contaminants.”
Binary planetary nebulae nuclei towards the Galactic bulge - I. Sample discovery, period distribution, and binary fraction (2009, methodology): “3.1) wellknown symbiotics were removed using SIMBAD and literature sources (Belczyński et al. 2000; Phillips 2007; Schmeja & Kimeswenger 2001).”
THE ASTRALUX LARGE M-DWARF MULTIPLICITY SURVEY (2012, background): “The X-ray flux of this star is probably due to the fact that it is a symbiotic star, as identified by, e.g., Belczynski et al. (2000), hence we consider it as a contaminant to the Riaz et al. (2006) sample.”
Dawes Review 6: The Impact of Companions on Stellar Evolution (2016, background): “…Heuvel 2006 Sequence E stars RGB and AGB stars with close companion Nicholls & Wood 2012 Symbiotic binaries WD accreting from an RGB or AGB giant Belczyński et al. 2000, Jorissen 2003 Wolf–Rayet + O binaries Massive Wolf–Rayet + O star binaries Gosset et al. 2001 Double degenerates Often…”