activity
20152020
most citedDistinguishing between symbiotic stars and planetary nebulae

29 citations · 56 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.SR20203 cited

Optical spectroscopy and X-ray observations of the D-type symbiotic star EF Aql

K. A. Stoyanov, K. Iłkiewicz, G. J. M. Luna +6

We performed high-resolution optical spectroscopy and X-ray observations of the recently identified Mira-type symbiotic star EF Aql. Based on high-resolution optical spectroscopy o…

astro-ph.GA2020

On the absence of symbiotic stars in globular clusters

Diogo Belloni, Joanna Mikołajewska, Krystian Iłkiewicz +4

Even though plenty of symbiotic stars (SySts) have been found in the Galactic field and nearby galaxies, not a single one has ever been confirmed in a Galactic globular cluster (GC…

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.SR20199 cited

LMC S154: the first Magellanic symbiotic recurrent nova

Krystian Ilkiewicz, Joanna Mikolajewska, Brent Miszalski +3

Classical nova outburst has been suggested for a number of extragalactic symbiotic stars, but in none of the systems has it been proven. In this work we study the nature of one of…

astro-ph.SR2019

Hen 3-160 - the first symbiotic binary with Mira variable S star

C. Galan, J. Mikolajewska, B. Monard +3

Hen 3-160 is reported in Belczynski et al.'s (2000) catalog as a symbiotic binary system with M7 giant donor. Using - and -band photometry collected over 20 years we have fou…

astro-ph.SR2018

Wind Roche Lobe Overflow as a way to make type Ia supernova from the widest symbiotic systems

Krystian Ilkiewicz, Joanna Mikolajewska, Krzysztof Belczynski +2

Symbiotic stars are interacting binaries with one of the longest orbital periods. Since they can contain a massive white dwarf with a high accretion rate they are considered a poss…