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The large and small scale properties of the intergalactic gas in the Slug Ly-alpha nebula revealed by MUSE HeII emission observations
Sebastiano Cantalupo, Gabriele Pezzulli, Simon J. Lilly +11
With a projected size of about 450 kpc at z~2.3, the Slug Ly-alpha nebula is a rare laboratory to study, in emission, the properties of the intergalactic gas in the Cosmic Web. Sin…
Synthetic nebular emission from massive galaxies II: ultraviolet-line diagnostics of dominant ionizing sources
Michaela Hirschmann, Stéphane Charlot, Anna Feltre +3
We compute synthetic optical and ultraviolet (UV) emission-line properties of galaxies in a full cosmological framework by coupling, in post-processing, new-generation nebular-emis…
The MUSE Hubble Ultra Deep Field Survey: XII. MgII emission and absorption in star-forming galaxies
Anna Feltre, Roland Bacon, Laurence Tresse +18
The physical origin of the near-ultraviolet MgII emission remains an under-explored domain, contrary to more typical emission lines detected in the spectra of star-forming galaxies…