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The Flare and Warp of the Young Stellar Disk Traced with LAMOST DR5 OB-type Stars

  • Authors: Yang Yu, 扬 于, Hai-Feng Wang, 海峰 王, Wen-Yuan Cui, 文元 崔, Lin-Lin Li, 林林 李, Chao Liu, 超 刘, Bo Zhang, 博 章, Hao Tian, 浩 田, Zhen-Yan Huo, 振燕 霍, Jie Ju, 洁 巨, Zhi-Cun Liu, 志存 柳, Fang Wen, 芳 温, Shuai Feng, 帅 冯

Yang Yu et al 2021 The Astrophysical Journal 922 .

  • Provider: AAS Journals

Caption: Figure 4.

The figure shows the OB-type star scale height distribution compared with the gas disk as a function of the radial distance. The red line is the north-side scale height, and the black line is the southern scale height. The green line is the Kalberla et al. (2007) southern scale height of the H I gas disk, while the blue rectangles and pentagram are also the Kalberla et al. (2007) northern H I thickness distribution. Yellow pentagrams correspond to the H2 results in Nakanishi & Sofue et al. (2006). The average slope of the scale height (h z ) versus distance (R) describing the strength of flaring is labeled in the bottom left.

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