BeschrijvingDistribution of molecular gas in 30 merging galaxies.jpg
English: Each of the colourful objects in this image illustrates one of 30 merging galaxies. The contours in the individual galaxies show the signal strength from carbon monoxide while the colour represents the motion of gas. Gas that is moving away from us appears red while the blue colour shows gas that is approaching. The contours together with the transition from red to blue indicate a gaseous disc that is rotating about the centre of the galaxy.
ALMA (ESO/NAOJ/NRAO)/SMA/CARMA/IRAM/J. Ueda et al.
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Each of the colourful objects in this image illustrates one of 30 merging galaxies. The contours in the individual galaxies show the signal strength from carbon monoxide while the colour represents the motion of gas. Gas that is moving away from us appears red while the blue colour shows gas that is approaching. The contours together with the transition from red to blue indicate a gaseous disc that is rotating about the centre of the galaxy.
Uniek ID van het originele document
uuid:5D20892493BFDB11914A8590D31508C8
Credit/Leverancier
ALMA (ESO/NAOJ/NRAO)/SMA/CARMA/IRAM/J. Ueda et al.
Bron
European Southern Observatory
Korte naam
Distribution of molecular gas in 30 merging galaxies