Figure 2 from The CIDA Variability Survey of Orion OB1. II. Demographics of the Young, Low-mass Stellar Populations

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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 2.

The outline of the CVSO survey area (green dashed-line rectangle) projected in galactic coordinates and overlaid on the large-scale structure of the Orion–Eridanus super bubble, as depicted schematically by Ochsendorf et al. (2015) in their Figure 1(d). The solid red lines map the dust structures, while the blue lines correspond to the rough outlines of gas structures traced by Hα emission (adapted from Ochsendorf et al. 2015).

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