Image Details

Choose export citation format:

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 5.

Before, during, and after eclipse 280″ × 280″ snapshots from DASCH photographic plates. Top row: 1937 eclipse, bottom row: 1981 eclipse. For visual comparison, in addition to the target (J0705+0612) we mark two stars of brightness similar to J0705+0612, source a (Gaia DR3 3152915773802913792, G = 13.01 mag, BP − RP = 0.70 mag) and source b (Gaia DR3 3152917212612801536, G = 12.43 mag, BP − RP = 1.32 mag). The bluer source a appears brighter on the photographic plates.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse