Astrophysical: FU Orionis stars

  • Publication
    A Multi-epoch, Multiwavelength Study of the Classical FUor V1515 Cyg Approaching Quiescence

    Historically, FU Orionis-type stars are low-mass, pre-main-sequence stars. The members of this class experience powerful accretion outbursts and remain in an...

  • Publication
    A Study of the Photometric and Spectroscopic Variations of the Prototypical FU Orionis-type Star V1057 Cyg

    Among the low-mass pre-main sequence stars, a small group called FU Orionis-type objects (FUors) are notable for undergoing powerful accretion outbursts. V1057...