David Hughes
David Hughes
David Hughes
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separation of nuclei<br />
0.3 - 10 kpc, <br />
white contours show<br />
CO emission from<br />
OVRO interferometry<br />
sizes < 300 pc<br />
i.e. high mass densities<br />
star formation<br />
ALMA resolution at 1.1mm<br />
0.05 arcsecs, 5 km baseline<br />
resolves ~ 70 pc at z~3<br />
Scale-bar represents 10 kpc