File:Side-on 3D view of the Per-Tau Shell, giant structure forming star-forming molecular clouds (with Sun).png
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[编辑]描述Side-on 3D view of the Per-Tau Shell, giant structure forming star-forming molecular clouds (with Sun).png |
English: This is a CROPPED PART(!) of a figure from the study. Screenshot was made via Okular & Spectacle. Description for the complete(!) figure below. See the source for the complete figure and more images.
"FIG. 2.— 3D views of the Per-Tau shell (for an interactive version of this figure click here a b . See Fig. 5 for more static visualizations). Plotted are density iso-surfaces at levels n = 5 cm−3 (grey) and n = 25 cm−3 (color), overlaid with our spherical shell model,radius Rs = 78 pc, distance from the sun d = 218 pc. The n = 25 cm−3 surfaces are colored by distance from the sun (blue-to-red). Upper-left: View from the sun (compare with Fig. 1). Upper-right: A side view of the region. Perseus and Taurus and their diffuse envelopes are arranged on two opposing sides of the Per-Tau shell. Lower-left: Another side view emphasizing the Tau Ring. The ellipse is the Tau Ring model (Appendix B). Lower-right: 2D density slices along the xy, xz, yz planes. All planes intersect at shell’s center. In all panels xyz are the Heliocentric Cartesian Galactic Coordinates. a URL address for the interactive figure: https://faun.rc.fas.harvard.edu/czucker/Paper Figures/sbialy/pertau superbubble.html. b For Augmented Reality (AR) experience, scan the QR codes with a mobile device (CoSpaces App required): Left code for viewing with a Merge Cube, right code for a tabletop AR. If you are already reading this article with a mobile device, click here (Merge Cube), or here (tabletop AR)." |
日期 | |
来源 | https://arxiv.org/abs/2109.09763v1 |
作者 | Authors of the study: Shmuel Bialy, Catherine Zucker, Alyssa Goodman, Michael M. Foley, João Alves, Vadim A. Semenov, Robert Benjamin, Reimar Leike, Torsten Enßlin |
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文件修改日期时间 | 2021年10月18日 (一) 20:31 |