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One of the most attractive events in the pre-main sequence evolution is theFU Orionis (FUor) outburst. Because only a small number of FUor stars have beendetected to date, photometric and spectral studies of every new object are ofgreat interest. Recently, a new FUor candidate was discovered by Anton Khruslov- V582 Aur. To confirm the FUors nature of this object we started regularphotometric observations with the telescopes of the National AstronomicalObservatory Rozhen (Bulgaria). A high-resolution spectrum of V582 Aur wasobtained with the 1.93 m telescope in Haute-Provence Observatory (France).

The FUor Candidate V582 Aurigae: First Photometric and Spectroscopic Observations