5 papers
Inside-Out vs. Outside-In Quenching of MaNGA Galaxies: Dependence on Stellar Mass and Environment
Zi-Hua Ho, Lihwai Lin, Hung-Yu Jian +6
Galaxy quenching, the cessation of star formation, can proceed in spatially distinct ways, commonly described as inside-out or outside-in. However, the inferred quenching pattern d…
The GECKOS survey: Resolving the molecular and ionised gas in the galactic outflow of ESO~484-036
J. Hernández-Yévenes, D. B. Fisher, B. Mazzilli Ciraulo +20
We present a spatially resolved, multiphase study of the outflow in the edge-on starburst galaxy ESO~484-036 from the GECKOS survey, combining VLT/MUSE H and ALMA CO(10) obs…
Physical properties of gas departing from circular rotation at 50 pc scales using the PHANGS-MUSE galaxies
Carlos López-Cobá, Lihwai Lin, Irene Cruz González +4
Noncircular motions have been observed across various spatial scales in disk galaxies, yet the physical properties of the gas involved in these motions remain poorly constrained. U…
On the role of non-circular motions in MaNGA galaxies I: global properties
Carlos Lopez-Coba, Lihwai Lin, Justus Neumann +1
Non-circular (NC) motions represent the imprints of non-axisymmetric structures in galaxies, providing opportunities to study the physical properties of gas departing from circular…
Do strong bars exhibit strong non-circular motions?
Taehyun Kim, Dimitri A. Gadotti, Yun Hee Lee +4
Galactic bars induce characteristic motions deviating from pure circular rotation, known as non-circular motions. As bars are non-axisymmetric structures, stronger bars are expecte…