86 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Crimean Astrophysical ObservatoryUA6 papers
- Kyoto UniversityJP6 papers
- Vihorlat ObservatorySK6 papers
- Hungarian Astronomical AssociationHU5 papers
- British Astronomical AssociationGB4 papers
- Osaka Kyoiku UniversityJP4 papers
- RIKENJP4 papers
- Swansea UniversityGB4 papers
- Universidad de HuelvaES4 papers
- American Association of Variable Star ObserversUS3 papers
- Institute of AstronomyRU3 papers
- International Center for Astronomical, Medical and Ecological ResearchUA3 papers
4 papers · 1 filter
On the nature of the anomalous event in 2021 in the dwarf nova SS Cygni and its multi-wavelength transition
Mariko Kimura, Shinya Yamada, Nozomi Nakaniwa +20
SS Cyg has long been recognized as the prototype of a group of dwarf novae that show only outbursts. However, this object has entered a quite anomalous event in 2021, which at firs…
Multi-wavelength photometry during the 2018 superoutburst of the WZ Sge-type dwarf nova EG Cancri
Mariko Kimura, Keisuke Isogai, Taichi Kato +45
We report on the multi-wavelength photometry of the 2018 superoutburst in EG Cnc. We have detected stage A superhumps and long-lasting late-stage superhumps via the optical photome…
Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. X: The Tenth Year (2017)
Taichi Kato, Keisuke Isogai, Yasuyuki Wakamatsu +67
Continuing the project described by Kato et al. (2009, PASJ, 61, S395, arXiv/0905.1757), we collected times of superhump maxima for 102 SU UMa-type dwarf novae observed mainly duri…
Discovery of Standstills in the SU UMa-Type Dwarf Nova NY Serpentis
Taichi Kato, Elena P. Pavlenko, Nikolaj V. Pit +40
We found that the SU UMa-type dwarf nova NY Ser in the period gap [orbital period 0.097558(6) d] showed standstills twice in 2018. This is the first clear demonstration of a stands…