Tomography of gas inflow into the central region of NGC 4051
Tomography of gas inflow into the central region of NGC 4051 showing velocity slices along the H2 profile with a velocity bin of ~42 kilometers/second. The cross indicates the position of the nucleus. The inflow along the nuclear spiral is observed in blueshift in the top panels and in redshift in the bottom panels.
Credit:International Gemini Observatory/NOIRLab/NSF/AURA
About the Image
Id: | geminiann08007a |
Type: | Collage |
Release date: | Feb. 20, 2008, 2:54 p.m. |
Related announcements: | geminiann08007 |
Size: | 500 x 615 px |