Hot gas, cold gas and sub-haloes in a Lyman α blob at redshift 2.38
We present integral field spectroscopy of a Lyman α blob at redshift 2.38, with a spectral resolution three times better than previous published work. As with previous observations, the blob has a chaotic velocity structure, much of which breaks up into
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Francis_Hot_gas,_cold_gas_and_2013.pdf||3.82 MB||Adobe PDF||Request a copy|
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