Image Details

Choose export citation format:

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 1.

The Orion OB1 association as studied by the CVSO. The most prominent and well-known stellar groups and nebulosity found across this extended region are labeled. Throughout this work, we assume the OB1b subassociation to be the area contained within the dashed-line circle roughly centered on ϵ Ori, as defined in Briceño et al. (2005). The OB1a subassociation is all the area west of the straight dashed lines and of OB1b. The B Cloud is considered here as the region east of the boundary with OB1a and OB1b, north of −2°, while the A Cloud is roughly the region east of 5h28m, south of −2°, and excluding OB1b (optical image courtesy of Rogelio Bernal Andreo, DeepSkyColors.com).

Other Images in This Article

Show More

Copyright and Terms & Conditions