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).

Créditos:

International Gemini Observatory/NOIRLab/NSF/AURA

About the Image

Id:geminiann05002b
Tipo:Simulation
Release date:23 de Febrero de 2005 a las 14:52
Related announcements:geminiann05002
Size:1542 x 485 px

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Categoría:Illustrations

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