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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 1.

The top figure shows the normalized number counts distribution of OB-type stars without considering selection effects during this work. The bottom one is the sky coverage of our OB-type stars adopted from Liu et al. (2019). The area of the sky is mainly the Galactic anticenter direction; the sample is mainly in the range l = [140° 210°], b = [−3°, 5°], with a relatively small contribution from other areas.

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