Shuai Zhang

Carbon stars are excellent kinematic tracers of galaxies and play important roles in understanding the evolution of the Galaxy. Therefore, it is worthwhile to search for them in a…

astro-ph.GA2016★ 26 cited

Molecular clouds and star formation toward the Galactic plane within 216.25 $^{o} \leq$ l $\leq$ 218.75 $^{o}$ and $-$ 0.75 $^{o} \leq$ b $\leq$ 1.25 $^{o}$

Y. Gong, R. Q. Mao, M. Fang +9

As a part of the Milky Way Imaging Scroll Painting (MWISP) survey, we performed a simultaneous 12CO(1-0), 13CO(1-0), C18O(1-0) mapping toward molecular clouds in a region encompass…

Identification of Carbon Stars from LAMOST DR7

Molecular clouds and star formation toward the Galactic plane within 216.25o≤ l ≤218.75o and −0.75o≤ b ≤1.25o

Molecular clouds and star formation toward the Galactic plane within 216.25 $^{o} \leq$ l $\leq$ 218.75 $^{o}$ and $-$ 0.75 $^{o} \leq$ b $\leq$ 1.25 $^{o}$