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The Emerging Stellar Complex in Mon R2: Membership and Optical Variability Classification

  • Authors: Sally D. Jiang, Lynne A. Hillenbrand

Sally D. Jiang and Lynne A. Hillenbrand 2024 The Astronomical Journal 167 .

  • Provider: AAS Journals

Caption: Figure 14.

Flux asymmetry (M) vs. quasiperiodicity (Q) plotted for our sample of 470 variable member sources. Primary variability classes are shown by the marker indicated in the legend. Sources with a secondary classification (multiperiodic or long timescale) are marked in addition to their primary class. The dotted lines show the limits in Q and M for the differing classes, with Q = 0.45 and Q = 0.82 dividing the periodic from quasiperiodic and quasiperiodic from stochastic sources, and M = −0.25 and M = +0.25 dividing the burster from symmetric and symmetric from dipper sources.

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