activity
20192022
most citedThe molecular gas resolved by ALMA in the low-metallicity dwarf merging galaxy Haro 11

15 citations · 34 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202215 cited

The molecular gas resolved by ALMA in the low-metallicity dwarf merging galaxy Haro 11

Yulong Gao, Qiusheng Gu, Yong Shi +9

The physical mechanisms for starburst or quenching in less massive () galaxies are unclear. The merger is one of the inescapable processes referred to as b…

astro-ph.GA20226 cited

Asymmetric star formation triggered by gas inflow in a barred lenticular galaxy PGC 34107

Shiying Lu, Qiusheng Gu, Xue Ge +8

Comparing to the inactive and gas-poor normal lenticular galaxies (S0s) in the local universe, we study a barred star-forming S0 galaxy, PGC 34107, which has been observed by the C…

astro-ph.GA20213 cited

Observations of cold gas and star formation in dwarf S0 galaxies

Xue Ge, Qiu-Sheng Gu, Ruben Garcıa-Benito +3

Very little work has been done on star formation in dwarf lenticular galaxies (S0s). We present 2D-spectroscopic and millimetre observations made by Centro Astronomico Hispano Alem…

astro-ph.GA202110 cited

The effect of the morphological quenching mechanism on star formation activity at 0.5 < z < 1.5 in 3D-HST/CANDELS

Shiying Lu, Guanwen Fang, Yizhou Gu +3

Several mechanisms for the transformation of blue star-forming to red quiescent galaxies have been proposed, and the green valley (GV) galaxies amid them are widely accepted in a t…

astro-ph.GA2020

Structures, stellar population properties, AGN fractions, and environments of massive compact galaxies at in 3D--{\it HST}/CANDELS

Yizhou Gu, Guanwen Fang, Qirong Yuan +1

We present a study on structures and physical properties of massive ($M_* >10^{10} M_{\sun} $) compact galaxies at in five 3D--{\it HST}/CANDELS fields. Compared with t…

astro-ph.GA2019

The mass dependence of structure, star formation rate, and mass assembly mode at 0.5<z< 2.5

Yizhou Gu, Guanwen Fang, Qirong Yuan +5

To investigate the mass dependence of structural transformation and star formation quenching, we construct three galaxy samples using massive () red, green…