GSC 08227-00723 is classified as a new AH Pic-type nova-like variable with recurrent stunted outbursts and an exceptionally large positive superhump excess of approximately 0.19.
Osaki, Publications of the Astronomical Society of th e Pacific 108, 39 (1996)
3 Pith papers cite this work. Polarity classification is still indexing.
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New photometry of RZ LMi and KV Dra detects superhumps during superoutbursts, determines periods and amplitudes, clarifies ER UMa and WZ Sge subclassifications, and measures a 0.0586-day orbital period for KV Dra.
Discovery of KSP-OT-202104a, a new WZ Sge-type dwarf nova with P_sh ≈ 71.7 min likely below the period minimum and evolving toward AM CVn.
citing papers explorer
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GSC 08227-00723: An Unusually Large PSH Excess AH Pic Candidate
GSC 08227-00723 is classified as a new AH Pic-type nova-like variable with recurrent stunted outbursts and an exceptionally large positive superhump excess of approximately 0.19.
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Photometric light curves analysis of SU UMa-type dwarf novae: the case of RZ LMi and KV Dra
New photometry of RZ LMi and KV Dra detects superhumps during superoutbursts, determines periods and amplitudes, clarifies ER UMa and WZ Sge subclassifications, and measures a 0.0586-day orbital period for KV Dra.
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A New WZ Sagittae-type Dwarf Nova KSP-OT-202104a Near the Period Minimum from the KMTNet Supernova Program
Discovery of KSP-OT-202104a, a new WZ Sge-type dwarf nova with P_sh ≈ 71.7 min likely below the period minimum and evolving toward AM CVn.