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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 5.

Left: vector point diagram of proper motion distributions among all Gaia DR3 stars over the 2.5 × 2.5 deg2 query area centered on Mon R2. The color bar indicates the astrometric membership probability (P astrom) as described in the text. Middle: stars with astrometric membership probability P astrom > 0.25. Right: field stars excluded from the candidate member sample as a result of low astrometric membership probability.

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