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TRAO Survey of Nearby Filamentary Molecular Clouds, the Universal Nursery of Stars (TRAO-FUNS). III. Filaments and Dense Cores in the NGC 2068 and NGC 2071 Regions of Orion B

  • Authors: Hyunju Yoo, Chang Won Lee, Eun Jung Chung, Shinyoung Kim, Mario Tafalla, Paola Caselli, Philip C. Myers, Kyoung Hee Kim, Tie Liu, Woojin Kwon, Archana Soam, Jongsoo Kim

Hyunju Yoo et al 2023 The Astrophysical Journal 957 .

  • Provider: AAS Journals

Caption: Figure 2.

The color scale presents a Herschel 250 μm continuum image of the Orion B region. Contours are from the integrated intensity maps of 13CO (middle left panel) and C18O (middle right panel). The contour levels for the 13CO integrated intensity map are [1, 3, 5, 7, 9, 11] K km s−1 and those for the C18O integrated intensity map are [0.25, 0.75, 1, 1.5, 2.2, 3.5, 6] K km s−1. Panels (a)–(f) show representative spectra of 13CO (black line) and C18O (blue line) at the central positions marked with green dots in the middle left panel and the middle right panel. In panel (a)–(f), the C18O spectrum is scaled up by a factor of 2 and shifted by –1 in intensity. The gray and cyan horizontal lines represent baselines of the 13CO and C18O spectra, respectively.

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