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1RXH J082623.6–505741: A New Long-period Cataclysmic Variable with an Evolved Donor and a Low Mass-transfer Rate

  • Authors: Kirill V. Sokolovsky, Jay Strader, Samuel J. Swihart, Elias Aydi, Arash Bahramian, Laura Chomiuk, Craig O. Heinke, Allison K. Hughes, Kwan-Lok Li, Raimundo Lopes de Oliveira, James C. A. Miller-Jones, Koji Mukai, David J. Sand, Laura Shishkovsky, Evangelia Tremou, Karina Voggel

Kirill V. Sokolovsky et al 2022 The Astrophysical Journal 934 .

  • Provider: AAS Journals

Caption: Figure 7.

Continuum-normalized moderate-resolution SOAR/Goodman spectrum taken on 2017-11-15. Double-peaked emission lines of He I at 5875 and 6678 Å and H I at 6563 Å from the accretion disk are evident, as are the numerous narrow metal absorption lines from the secondary. The resonance Na I line is a blend of absorption from the secondary and the interstellar medium.

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