2 papers
astro-ph.SR2020
Molecular remnant of Nova 1670 (CK Vulpeculae). II. A three-dimensional view on the gas distribution and velocity field
T. Kamiński, W. Steffen, V. Bujarrabal +3
CK Vul is the remnant of an energetic eruption known as Nova 1670 that is thought to be caused by a stellar merger. The remnant is composed of (1) a large hourglass nebula of recom…
astro-ph.SR2018
ALMA reveals the aftermath of a white dwarf--brown dwarf merger in CK Vulpeculae
Stewart Eyres, Aneurin Evans, Albert Zijlstra +7
We present Atacama Large Millimeter-Submillimeter Array (ALMA) observations of CK Vulpeculae which is identified with "Nova Vulpeculae 1670". They trace obscuring dust in the inner…