Nuclear ashes and outflow in the eruptive star Nova Vul 1670

@article{Kamiski2015NuclearAA,
  title={Nuclear ashes and outflow in the eruptive star Nova Vul 1670},
  author={T. Kamiński and K. Menten and R. Tylenda and M. Hajduk and N. Patel and A. Kraus},
  journal={Nature},
  year={2015},
  volume={520},
  pages={322-324}
}
CK Vulpeculae was observed in outburst in 1670–1672 (ref. 1), but no counterpart was seen until 1982, when a bipolar nebula was found at its location. Historically, CK Vul has been considered to be a nova (Nova Vul 1670), but its similarity to ‘red transients’, which are more luminous than classical novae and thought to be the results of stellar collisions, has re-opened the question of CK Vul’s status. Red transients cool to resemble late M-type stars, surrounded by circumstellar material rich… Expand
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