2021/07/30 by Taichi Kato, Kato, Taichi, Naoto Kojiguchi +1
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysical Phenomena and Observations #FOS: Physical sciences #Gamma-ray bursts and supernovae #High-pressure geophysics and materials #Solar and Stellar Astrophysics (astro-ph.SR)
paper · pdf · doi:10.48550/arxiv.2107.14400
openalex publication_date 2021/07/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Using Public Data Release of Zwicky Transient Facility observations, we found that MGAB-V859 and ZTF18abgjsdg are dwarf novae and show both ER UMa-type and Z Cam-type states. There had been only two dwarf novae showing similar transitions between the ER UMa-type and Z Cam-type states. MGAB-V859 showed both a transition from the ER UMa-type state to a long standstill in 2019 and a Z Cam-type state in 2020. During the standstill in 2020, this object faded twice and showed dwarf nova-type variations. ZTF18abgjsdg usually showed ER UMa-type behavior but standstills were seen in 2018 and 2019. The supercycles of these objects during the typical ER UMa-type phase were 55 d and 58 d, respectively. These objects provide additional evidence that some ER UMa stars indeed bridge between dwarf nova and novalike states as proposed in Kato et al. (2016).