The structure of a recent nova shell as observed by ALMA
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY(2018)
摘要
High resolution ALMA observations of the recent (2.52 yr old) shell of Nova V5668 Sgr (2015) show a highly structured ionized gas distribution with small (10(15) cm) clumps. These are the smallest structures ever observed in the remnant of a stellar thermonuclear explosion. No extended contiguous emission could be found above the 2.5 sigma level in our data, while the peak hydrogen densities in the clumps reach 10(6) cm(-3). The millimetre continuum image suggests that large scale structures previously distinguished in other recent nova shells may result from the distribution of bright unresolved condensations.
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关键词
stars: novae, cataclysmic variables,stars: white dwarfs,radio continuum: stars
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