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ASASSN-24fw: Candidate Gas-rich Circumsecondary Disk Occultation of a Main-sequence Star

  • Authors: Nadia L. Zakamska, Gautham Adamane Pallathadka, Dmitry Bizyaev, Jaroslav Merc, James E. Owen, Henrique Reggiani, Kevin C. Schlaufman, Karolina Bąkowska, Sławomir Bednarz, Krzysztof Bernacki, Agnieszka Gurgul, Kirsten R. Hall, Franz-Josef Hambsch, Barbara Joachimczyk, Krzysztof Kotysz, Sebastian Kurowski, Alexios Liakos, Przemysław J. Mikołajczyk, Erika Pakštienė, Grzegorz Pojmański, Adam Popowicz, Daniel E. Reichart, Łukasz Wyrzykowski, Justas Zdanavičius, Michał Żejmo, Paweł Zieliński, Staszek Zola

Nadia L. Zakamska et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 9.

Balmer series lines Hα, Hβ, and Hγ as seen by GHOST compared with the low-metallicity BOSZ templates. The bottom curve shows Hα after subtraction of the BOSZ template and a two-Gaussian fit to the emission profile. No rotational broadening was applied to the template as these lines are intrinsically broad.

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