Abstract
Aims. We present an analysis of a peculiar supergiant B-type star (VFTS698/Melnick 2/Parker 1797) in the 30 Doradus region of the Large Magellanic Cloud which exhibits characteristics similar to the broad class of B[e] stars. Methods. We analyse optical spectra from the VLT-FLAMES survey, together with archival optical and infrared photometry and X-ray imaging to characterise the system. Results. We find radial velocity variations of around 400 km s -1 in the high excitation Si iv, N iii and He ii spectra, and photometric variability of ∼0.6 mag with a period of 12.7 d. In addition, we detect long-term photometric variations of ∼0.25 mag, which may be due to a longer-term variability with a period of ∼400 d. Conclusions. We conclude that VFTS698 is likely an interacting binary comprising an early B-type star secondary orbiting a veiled, more massive companion. Spectral evidence suggests a mid-to-late B-type primary, but this may originate from an optically-thick accretion disc directly surrounding the primary.
| Original language | English |
|---|---|
| Article number | A50 |
| Journal | Astronomy and Astrophysics |
| Volume | 542 |
| DOIs | |
| Publication status | Published - 2012 |
Keywords
- Be
- Binaries: spectroscopic
- Stars: early-type
- Stars: emission-line
- Stars: peculiar
- Stars: variables: general
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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