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Value-added Catalogs of M-type Stars in LAMOST DR5

  • Authors: Jing Zhong, Jing Li, Jeffrey L. Carlin, Li Chen, Rene A. Mendez, and Jinliang Hou

2019 The Astrophysical Journal Supplement Series 244 8.

  • Provider: AAS Journals

Caption: Figure 9.

Toomre density diagram of confirmed M giants. The red line kinematically divides the M giants sample into halo and disk components, since stars with ∣VVLSR∣ > 180 km s−1 have higher probabilities of being members of the Galactic halo.

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