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A New WZ Sagittae-type Dwarf Nova KSP-OT-202104a Near the Period Minimum from the KMTNet Supernova Program

  • Authors: Sang Chul Kim, Youngdae Lee, Dae-Sik Moon, Hong Soo Park, Yuan Qi Ni, Nan Jiang, Hyobin Im

Sang Chul Kim et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 7.

Gemini spectrum of KSP-OT-202104a obtained by combining blue and red spectra shown after 16 Å smoothing. Extinction is not corrected. The locations of H and He lines often observed in WZ Sge-type DNe are marked by vertical lines: solid, dotted, and dashed lines for H I, He I, and He II, respectively. They are Hα (6563 Å), Hβ (4861 Å), Hγ (4340 Å), Hδ (4102 Å), Hϵ (3970 Å), Hζ (3889 Å), He I (red), and He II (black), while wavelengths are shown for helium lines.

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