High-resolution mapping reveals nitrogen enrichment around super star clusters in NGC 5253, attributed to Wolf-Rayet stars with material expelled to surrounding gas.
@doi [Science] 10.1126/science.ado9787, https://ui.adsabs.harvard.edu/abs/2025Sci...387.1209Z 387
4 Pith papers cite this work. Polarity classification is still indexing.
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GSED unifies six heterogeneous 3D extinction datasets into a single homogenized catalogue of over 1.9 billion entries via a six-layer MLP and provides a real-time coordinate-based query service.
HETDEX PDR1 releases an expanded public catalog of 426,654 LAEs, 491,411 [O II] emitters and additional sources from 86.67 sq deg of integral-field spectroscopy with improved classifiers.
The Galactic Center Lobe is a foreground HII region at ~2 kpc, photoionized and forming a closed outer loop, not a Galactic center feature.
citing papers explorer
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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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GSED: The Galactic Stellar Extinction Database
GSED unifies six heterogeneous 3D extinction datasets into a single homogenized catalogue of over 1.9 billion entries via a six-layer MLP and provides a real-time coordinate-based query service.
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HETDEX Public Data Release 1: Source Catalog 2 and Data Cubes from ~90 sq deg of Integral-Field Optical Spectroscopy
HETDEX PDR1 releases an expanded public catalog of 426,654 LAEs, 491,411 [O II] emitters and additional sources from 86.67 sq deg of integral-field spectroscopy with improved classifiers.
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SDSS-V LVM: Verifying what, and where, the 'Galactic Center' Lobe is
The Galactic Center Lobe is a foreground HII region at ~2 kpc, photoionized and forming a closed outer loop, not a Galactic center feature.