Corpus ID: 118587091

Review Of The 2010 Eruption Of Recurrent Nova U Scorpii

  title={Review Of The 2010 Eruption Of Recurrent Nova U Scorpii},
  author={B. Schaefer},
  journal={arXiv: Solar and Stellar Astrophysics},
  • B. Schaefer
  • Published 2010
  • Physics
  • arXiv: Solar and Stellar Astrophysics
On 28 January 2010, the recurrent nova U Scorpii had its long predicted eruption; prior preparation allowed for this to become the all-time best observed nova event. The coverage included daily and hourly spectra in the X-ray, ultraviolet, optical, and infrared, plus daily and hourly photometry in the X-ray, ultraviolet, U, B, V, y, R, I, J, H, K, and middle infrared, including roughly 35,000 V-band magnitudes (an average of better than once every three minutes) throughout the entire 67 days of… Expand