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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…
Molecular remnant of Nova 1670 (CK Vulpeculae): I. Properties and enigmatic origin of the gas
T. Kaminski, K. M. Menten, R. Tylenda +5
CK Vul erupted in 1670 and is considered a stellar-merger candidate. Its remnant contains a molecular component of surprisingly rich composition. We present interferometric line su…
SiO maser astrometry of the red transient V838 Monocerotis
Gisela N. Ortiz-Leon, Karl M. Menten, Tomasz Kaminski +3
We present multi-epoch observations with the VLBA of SiO maser emission in the v=1, J=1-0 transition at 43 GHz from the remnant of the red nova V838 Mon. We model the positions of…