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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 3.

Photometry from SkyMapper, 2MASS, and WISE. Blue: Planck spectrum (dark blue) and the BOSZ template (lighter blue) corresponding to our measured stellar parameters for J0705+0612. Red: the best-fit disk model from M. Jura (2003) with parameters as labeled (dashed line), with the full photosphere + disk fit shown in the solid line. Inclination angle i is the angle between the disk axis and the observer’s line of sight, so ﹩\cos i=1﹩ would correspond to a face-on orientation and maximal brightness.

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