The pre-main-sequence star V1184 Tauri (CB 34V) at the end of prolonged eclipse
E. H. SemkovInstitute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences, 72 Tsarigradsko Shose Blvd., 1784 Sofia, BulgariaS. P. PenevaInstitute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences, 72 Tsarigradsko Shose Blvd., 1784 Sofia, BulgariaS. I. IbryamovDepartment of Theoretical and Applied Physics, Faculty of Natural Sciences, University of Shumen, 115 Universitetska Str., 9712 Shumen, Bulgaria
2015en
ABI
Аннотация
Aims. V1184 Tau (CB 34V) lies in the field of the Bok globule CB 34 and was discovered as a large amplitude variable in 1993. According to the first hypothesis of the variability of the star, it is a FU Orionis candidate erupted between 1951 and 1993. During subsequent observations, the star manifests large amplitude variability interpreted as obscuration from circumstellar clouds of dust. We included V1184 Tau (CB 34V) in our target list of highly variable pre-main-sequence stars to determine the reasons for the variations in the brightness of this object.
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