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The CIDA Variability Survey of Orion OB1. II. Demographics of the Young, Low-mass Stellar Populations

  • Authors: César Briceño, Nuria Calvet, Jesús Hernández, A. Katherina Vivas, Cecilia Mateu, Juan José Downes, Jaqueline Loerincs, Alice Pérez-Blanco, Perry Berlind, Catherine Espaillat, Lori Allen, Lee Hartmann, Mario Mateo, and John I. Bailey III

2019 The Astronomical Journal 157 85.

  • Provider: AAS Journals

Caption: Figure 18.

Overdensities of candidate PMS sources in the OB1a region surrounding the 25 Ori cluster. The grayscale map is the surface density of photometric candidate PMS sources selected from the CVSO photometric survey based on their location in the PMS locus of the V vs. V − J CMD and detected as variable in the optical bands. Red stars correspond to early-type stars of B1–B2 spectral type, red triangles to B3–B5 stars, and magenta dots to B6–B9 stars. We have highlighted the B2 stars 25 Ori, HR 1833, and HD 35672 with large blue stars.

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