2010/08/23 by E. Semkov, Semkov, Evgeni, Stoyanka Peneva +3
Engineering · Physics and Astronomy · #Astro and Planetary Science #Astronomical Observations and Instrumentation #FOS: Physical sciences #Solar and Stellar Astrophysics (astro-ph.SR) #Stellar, planetary, and galactic studies
paper · pdf · doi:10.48550/arxiv.1008.3899
openalex publication_date 2010/08/23 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
One of the most attractive events in the pre-main sequence evolution is the FU Orionis (FUor) outburst. Because only a small number of FUor stars have been detected to date, photometric and spectral studies of every new object are of great interest. Recently, a new FUor candidate was discovered by Anton Khruslov - V582 Aur. To confirm the FUors nature of this object we started regular photometric observations with the telescopes of the National Astronomical Observatory Rozhen (Bulgaria). A high-resolution spectrum of V582 Aur was obtained with the 1.93 m telescope in Haute-Provence Observatory (France).