Table 1
Morphology types in the light curve sample of NGC 2264 members.
Morphology class | Count | c/w | % tot. | % Per |
|
||||
Burster | 21 | 21/0 | 4.2 | 38.1 |
Dipper | 37 | 35/0 | 7.4 | 68.6 |
Spotted | 187 | 44/153 | 37.3 | 100.0 |
Multi-periodic | 34 | 6/24 | 7.2 | 100.0 |
Eclipsing binary | 3 | 2/1 | 0.6 | 100.0 |
Stochastic | 22 | 19/0 | 4.4 | 31.6 |
Long-timescale variable | 3 | 2/1 | 0.6 | 33.3 |
Non-variable | 82 | 20/40 | 16.3 | 0.0 |
Others* | 114 | 27/58 | 22.7 | 28.7 |
Notes. Morphology class = classification of the light curve variability type; each class is briefly defined in Appendix A of this work. Count = number of objects in the sample with light curves falling in the corresponding category (a given object is here attributed to a single category, namely the one that best describes the dominant variability features of its light curve, although some cases may also exhibit traits of a different morphology class). c/w = number of CTTS/number of WTTS among objects in the corresponding morphology class. % tot. = percentage of objects in the sample that fall in the corresponding morphology class. % Per = percentage of objects in the corresponding morphology class which are found to be periodic.
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