Photometric behaviour of the FU Orionis type star, V1057 Cygni, during the last 25 years
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/434/1/38/18751582/stt963.pdf
Reference51 articles.
1. Long-term evolution of FU Orionis objects at infrared wavelengths
2. A search for Keplerian periods in the brightness variations of T Tauri and Ae Herbig stars
3. THE NATURE AND EVOLUTIONARY STATE OF THE FU ORIONIS BINARY SYSTEM
4. First astronomical unit scale image of the GW Orionis triple system
5. A binary origin for FU Orionis stars
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2. Multiwavelength detection of an ongoing FUOr-type outburst on a low-mass YSO;Monthly Notices of the Royal Astronomical Society: Letters;2023-12-27
3. Three-dimensional SPH Simulations of FU Orionis Star Flares in the Clumpy Accretion Model;The Astrophysical Journal;2023-08-01
4. Magnetically activated accretion outbursts of pre-main-sequence discs;Monthly Notices of the Royal Astronomical Society;2023-06-14
5. The FUor Star V2493 Cyg (HBC 722)—Eleven Years at Maximum Brightness;Symmetry;2021-12-16
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