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Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon III. HD 50138
Autoři | |
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Rok publikování | 2016 |
Druh | Článek v odborném periodiku |
Časopis / Zdroj | Astronomy and Astrophysics |
Fakulta / Pracoviště MU | |
Citace | |
Doi | http://dx.doi.org/10.1051/0004-6361/201526290 |
Obor | Astronomie a nebeská mechanika, astrofyzika |
Klíčová slova | circumstellar matter; stars: emission line Be; stars: mass loss; binaries: spectroscopic; stars: individual: MWC 158 |
Popis | We describe the spectral variability of HD 50138 over the last twenty years. Based on these data, we determine new restrictions for future modelling. We confirm the quasi-periodic behaviour of the object’s spectral variability, which probably reflects mass transfer in a binary system. This behaviour also supports a recently introduced explanation of the nature of FS CMa stars as post-merger systems. |