Large X-Ray Flare from the Herbig Be Star MWC 297

@article{Hamaguchi2000LargeXF,
  title={Large X-Ray Flare from the Herbig Be Star MWC 297},
  author={K. Hamaguchi and H. Terada and A. Bamba and K. Koyama},
  journal={The Astrophysical Journal},
  year={2000},
  volume={532},
  pages={1111-1118}
}
Hard X-ray emissions from the Herbig Be star MWC 297 were discovered in three separate observations spanning 5 days in 1994 April with the Advanced Satellite for Cosmology and Astrophysics (ASCA). An X-ray flare was found at the beginning of the second observation with a maximum luminosity of ≈4.9 × 1032 ergs s-1, which is 5 times larger than that of the quiescent phase (the first observation). It then declined with an e-folding time of ≈5.6 × 104 s to the preflare level in the third… Expand

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