He II Emission in Lyα Nebulae: Active Galactic Nucleus or Cooling Radiation?
We present a study of an extended Lyα nebula located in a known overdensity at z ∼ 2.38. The data include multiwavelength photometry covering the rest-frame spectral range from 0.1 to 250μm, and deep optical spectra of the sources associated with the
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|Source:||Astrophysical Journal, The|
|01_Scarlata_He_II_Emission_in_Lyα_Nebulae:_2009.pdf||778.37 kB||Adobe PDF||Request a copy|
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