Searching for periodicities in the MACHO light curve of LMC X-2
Using the exceptional long-term monitoring capabilities of the MACHO project, we present here the optical history of LMC X-2 for a continuous 6-yr period. These data were used to investigate the previously claimed periodicities for this source of 8.15 h and 12.54 d: we find upper limits of 0.10 mag...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2000-08, Vol.316 (4), p.729-733 |
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| creator | Alcock, C. Allsman, R. A. Alves, D. R. Axelrod, T. S. Becker, A. C. Bennett, D. P. Charles, P. A. Cook, K. H. Drake, A. J. Freeman, K. C. Geha, M. Griest, K. Groot, P. Lehner, M. J. Marshall, S. L. McGowan, K. E. Minniti, D. Nelson, C. A. Peterson, B. A. Popowski, P. Pratt, M. R. Quinn, P. J. Sutherland, W. Tomaney, A. B. Vandehei, T. van Paradijs, J. |
| description | Using the exceptional long-term monitoring capabilities of the MACHO project, we present here the optical history of LMC X-2 for a continuous 6-yr period. These data were used to investigate the previously claimed periodicities for this source of 8.15 h and 12.54 d: we find upper limits of 0.10 mag and 0.09 mag, respectively. |
| doi_str_mv | 10.1046/j.1365-8711.2000.03511.x |
| format | Article |
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| subjects | binaries: close stars: individual: LMC X-2 X-rays: stars |
| title | Searching for periodicities in the MACHO light curve of LMC X-2 |
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