High-resolution mapping reveals nitrogen enrichment around super star clusters in NGC 5253, attributed to Wolf-Rayet stars with material expelled to surrounding gas.
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A HeII-based correction method makes UV and optical measurements of electron temperature and O/H metallicity agree within 0.1 dex in three nearby BCD galaxies.
A homogeneous analysis of 699 spectra yields Te-Te relations for ions including N II, O II, O III, S II, S III and Ar III, with lower dispersions for relations involving Te([N II]).
Overview of HI modeling methods finds consistency in cosmic HI density but systematic differences in HI-halo mass relation shape and redshift evolution.
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The heart of NGC 5253 as seen with MUSE-NFM: nitrogen enrichment through stellar chemical feedback at parsec scales
High-resolution mapping reveals nitrogen enrichment around super star clusters in NGC 5253, attributed to Wolf-Rayet stars with material expelled to surrounding gas.
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Consistent Gas-Phase Temperatures and Metallicities from UV and Optical Nebular Emission: A Reliable Foundation from z=0 to Cosmic Dawn
A HeII-based correction method makes UV and optical measurements of electron temperature and O/H metallicity agree within 0.1 dex in three nearby BCD galaxies.
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The DESIRED electron temperature relations in star-forming regions of the local Universe
A homogeneous analysis of 699 spectra yields Te-Te relations for ions including N II, O II, O III, S II, S III and Ar III, with lower dispersions for relations involving Te([N II]).
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HI Simulations for Cosmology with the SKA Observatory
Overview of HI modeling methods finds consistency in cosmic HI density but systematic differences in HI-halo mass relation shape and redshift evolution.