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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 6.

Procedures identifying velocity-coherent filamentary structures with the FoF algorithm in the Orion B region. The colored regions denote the filamentary structures identified from FoF with the criteria for spatial separation (﹩\sqrt{2}﹩ pixel size) and velocity difference V diff (from 0.1–0.045 km s−1) written on the bottom of the panels. The gray region in each panel is a continuously connected structure within the velocity criteria and the shades (darker regions) in the gray region indicate that there are multiple velocity components in the line of sight in the velocity-coherent structure. The insets in the panels denote C18O (1–0) spectra and their decomposed Gaussian components at a pixel point. The numbers in the insets indicate the velocity centroids of the Gaussian components at the start point of the arrow. The colors of the velocity centroid numbers and Gaussian-fit profiles correspond to the colors of the filamentary structures.

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