9 citations · 16 across the 4 of their papers we have counts for
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Properties of Interstellar Medium in the S0 Galaxy NGC 1222: Evidence for Shocked-enhanced Line Emission
Jiamin Liu, Yinghe Zhao, Kai-Xing Lu +1
In this paper we present a comprehensive study on the properties of the interstellar medium in NGC~1222, a star-forming early-type merging galaxy that forms a triple system, using…
Metallicity dependence of the CO-to-H and the [CI]-to-H conversion factors in galaxies
Thomas G. Bisbas, Zhi-Yu Zhang, Maria-Christina Kyrmanidou +6
Understanding the molecular gas content in the interstellar medium (ISM) is crucial for studying star formation and galaxy evolution. The CO-to-H () and the [CI]-to…
Ionized Carbon in Galaxies: The [C II] 158 m Line as a Total Molecular Gas Mass Tracer Revisited
Yinghe Zhao, Jiamin Liu, Zhi-Yu Zhang +1
In this paper we present a statistical study of the [C II] 158 m line and the CO(1-0) emission for a sample of 200 local and high- (32 sources with ) galaxies with…
-enhanced Astrochemistry: the Carbon cycle in extreme galactic conditions
Thomas G. Bisbas, Zhi-Yu Zhang, Eda Gjergo +8
Astrochemistry has been widely developed as a power tool to probe physical properties of the interstellar medium (ISM) in various conditions of the Milky Way (MW) Galaxy, and in ne…