The expanding fireball of Nova Delphini 2013

@article{Schaefer2014TheEF,
  title={The expanding fireball of Nova Delphini 2013},
  author={Gail H. Schaefer and Theo A. ten Brummelaar and Douglas R. Gies and Christopher D. Farrington and Brian Kloppenborg and Olivier Chesneau and John D. Monnier and Stephen T. Ridgway and Nicholas J. Scott and I. Tallon-Bosc and Harold A. Mcalister and Tabetha Boyajian and Vicente Maestro and Denis Mourard and Anthony Meilland and Nicolas Nardetto and P. Stee and Judit Sturmann and Norm Vargas and F. Baron and Michael J. Ireland and Ellyn K. Baines and Xiao Che and J. M. Jones and Noel D. Richardson and Rachael M. Roettenbacher and Laszlo Sturmann and Nils H. Turner and Peter G. Tuthill and Gerard T. van Belle and Kaspar von Braun and Robert T. Zavala and Dipankar Banerjee and Nagarhalli M. Ashok and V. Joshi and Juliette C. Becker and Philip S. Muirhead},
  journal={Nature},
  year={2014},
  volume={515},
  pages={234-236}
}
A classical nova occurs when material accreting onto the surface of a white dwarf in a close binary system ignites in a thermonuclear runaway. Complex structures observed in the ejecta at late stages could result from interactions with the companion during the common-envelope phase. Alternatively, the explosion could be intrinsically bipolar, resulting from a localized ignition on the surface of the white dwarf or as a consequence of rotational distortion. Studying the structure of novae during… Expand
A nova outburst powered by shocks
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Explosive lithium production in the classical nova V339 Del (Nova Delphini 2013)
TLDR
The detection of highly blue-shifted resonance lines of the singly ionized radioactive isotope of beryllium, 7Be, in the near-ultraviolet spectra of the classical nova V339 Del (Nova Delphini 2013) 38 to 48 days after the explosion supports the theoretical prediction that a significant amount of 7Li is produced in classicalNova explosions. Expand
Multiwavelength models SED of the classical nova V339 Del (Nova Del 2013) along its age
Classical nova V339 Del (Nova Del 2013) is a fast nova of the Fe II class, whose eruption was ignited on a CO white dwarf (WD). In this contribution we present the spectral energy distribution (SED)Expand
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Context. Classical novae are the product of thermonuclear runaway-initiated explosions occurring on accreting white dwarfs. Aims. V339 Del (Nova Delphinus 2013) was one of the brightest classicalExpand
Multiwavelength Modeling of the SED of Nova V339 Del: Stopping the Wind and Long-lasting Super-Eddington Luminosity with Dust Emission
  • A. Skopal
  • Physics
  • The Astrophysical Journal
  • 2019
During the classical nova outburst, the radiation generated by the nuclear burning of hydrogen in the surface layer of a white dwarf (WD) is reprocessed by the outer material into different forms atExpand
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Radiative shocks create environments for dust formation in classical novae
Classical novae commonly show evidence of rapid dust formation within months of the outburst. However, it is unclear how molecules and grains are able to condense within the ejecta, given theExpand
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