International Gemini Observatory/NOIRLab/NSF/AURA
GMOS-South Probes Gas and Stellar Dynamics in Post-Merger Galaxy
Continuum (4900 – 5400 Å) image of “E+A” reconstructed by collapsing the IFU data (left). Middle panel shows the ionized gas ([OII] line intensity) and right panel shows the A stars distribution. Contours on center and right are those of the continuum light (from left panel).
