Polycyclic aromatic hydrocarbon emission within Lyα blobs
We present Spitzer observations of Lyα blobs (LABs) at z = 2.38-3.09. The mid-infrared ratios (4.5 μm/8 μm and 8 μm/24 μm) indicate that ∼60% of LAB infrared counterparts are cool, consistent with their infrared output being dominated by star forma
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Colbert_Polycyclic_aromatic_2011.pdf||503.92 kB||Adobe PDF|
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