A peculiar interacting be star binary in the small magellanic cloud

HIGHLIGHTS

  • who: Ronald E. Mennickent and colleagues from the Facultad de Ciencias Astronómicas y Geofísicas, Universidad de La Plata, Argentina have published the article: A Peculiar Interacting Be Star Binary in the Small Magellanic Cloud, in the Journal: (JOURNAL)
  • what: Based on the study of 17.5 years of I- and V-band OGLE photometry and new X-SHOOTER spectra we find that OGLEJ005039.05-725751.4 is very likely a binary consisting of a Be star in an eccentric orbit with orbital period 141.45 days.

SUMMARY

    Spectroscopic observations . . .

     

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