Ultraviolet emission from main-sequence companions of AGB stars

@article{Ortiz2016UltravioletEF,
  title={Ultraviolet emission from main-sequence companions of AGB stars},
  author={R. Ortiz and M. Guerrero},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2016},
  volume={461},
  pages={3036-3046}
}
  • R. Ortiz, M. Guerrero
  • Published 2016
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • Although the majority of known binary Asymptotic Giant Branch (AGB) stars are symbiotic systems (i.e. with a WD as a secondary star), main-sequence companions of AGB stars can be more numerous, even though they are more difficult to find because the primary high luminosity hampers the detection of the companion at visual wavelengths. However, in the ultraviolet the flux emitted by a secondary with T eff > 5500 ~ 6000 K may prevail over that of the primary, and then it can be used to search for… CONTINUE READING
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