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20122026
most citedConfirmation of the link between central star binarity and extreme abundance discrepancy factors in planetary nebulae

90 citations · 319 across the 13 of their papers we have counts for

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astro-ph.SR2026

K 1-6 is a photoionised ISM nebula shaped by a fast-moving hot white dwarf in a triple system

Jaroslav Merc, David Jones, Ana Escorza +22

K 1-6 has long been classified as a planetary nebula (PN) hosting a binary central star, yet it has remained poorly studied due to its faintness. The central star exhibits pronounc…