Abstract
We present a ∼5-yr optical light curve of the recurrent Be/X-ray transient A0538-66 obtained as a by-product of the MACHO Project. These data reveal both a long-term modulation at P = 420.8 ± 0.8 d and a short-term modulation at 16.6510 ± 0.0022 d which, within errors, confirms the previously found orbital period. Furthermore, the orbital activity is only seen at certain phases of the 421-d cycle, suggesting that the long-term modulation is related to variations in the Be star envelope.
Original language | English |
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Pages (from-to) | 678-684 |
Number of pages | 7 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 321 |
Issue number | 4 |
DOIs | |
Publication status | Published - 11 Mar 2001 |
Keywords
- Binaries: Close
- Stars: Individual: A0538-66
- X-rays: Stars
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science