Abstract :
[en] HD 50138 is a 6.6 mag emission-line B–type star, whose nature is still controversial. It has been thought to be a pre-main-sequence Herbig Be star and an evolved object with the B[e] phenomenon, possibly a mass-transferring binary system. However, it has mostly been studied on short timescales. We collected ∼1000 medium- and high-resolution spectra and available optical photometric data, which cover a time frame from 1981 to 2025, and extended the study from emission lines to a range of absorption lines. A few episodes of dramatic emission-line strength variations were uncovered as well as fast variations of the absorption line widths on timescales of several days. We also found a few previously unreported fadings of the star’s optical brightness seemingly associated with the Hα line profile changes. At the same time, it is still unclear whether the object is a single star or a binary system, as no regular variations of its observed parameters have been detected.
Funding text :
The work is carried out within the framework of the Project No. BR24992759 Development of the concept for the first Kazakhstani orbital cislunar telescope—Phase I, financed by the Ministry of Science and Higher Education of the Republic of Kazakhstan. This research was funded by the
Science Committee of the Ministry of Education and Science of the Republic of Kazakhstan (Grant No. AP19175392). S.Z. acknowledges PAPIIT grants IN102120 and IN119323.
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