Jixing Ge

most citedATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- VIII. A search for hot cores by using C

_{2}

_{5}

CN, CH

_{3}

OCHO and CH

_{3}

OH lines

42 citations · 42 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2024

Can near-to-mid infrared spectral energy distribution quantitatively trace protoplanetary disk evolution?

Mingchao Liu, Jinhua He, Zhen Guo +2

Infrared (IR) spectral energy distribution (SED) is the major tracer of protoplanetary disks. It was recently proposed to use the near-to-mid IR (or K-24) SED slope $α$ defined bet…

astro-ph.GA2022

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- X. Chemical differentiation among the massive cores in G9.62+0.19

Y. P. Peng, T. Liu, S. -L. Qin +23

Investigating the physical and chemical structures of massive star-forming regions is critical for understanding the formation and the early evolution of massive stars. We performe…

astro-ph.GA2022★ 42 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- VIII. A search for hot cores by using C $_{2}$ H $_{5}$ CN, CH $_{3}$ OCHO and CH $_{3}$ OH lines

Sheng-Li Qin, Tie Liu, Xunchuan Liu +29

Hot cores characterized by rich lines of complex organic molecules are considered as ideal sites for investigating the physical and chemical environments of massive star formation.…

Can near-to-mid infrared spectral energy distribution quantitatively trace protoplanetary disk evolution?

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- X. Chemical differentiation among the massive cores in G9.62+0.19

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- VIII. A search for hot cores by using C2​H5​CN, CH3​OCHO and CH3​OH lines

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- VIII. A search for hot cores by using C $_{2}$ H $_{5}$ CN, CH $_{3}$ OCHO and CH $_{3}$ OH lines