Aller au contenu principal
Accès ouvert déclaré 2026 article

Bright [C II ]158 μ m Streamers as a Beacon for Giant Galaxy Formation in SPT2349-56 at z = 4.3

2Citations signalées — pas une note de qualité
0Institutions déclarées
0Pays d’affiliation déclarés

Résumé fourni par la source

Abstract Observations of extreme starbursts, often located in the cores of protoclusters, challenge the classical bottom-up galaxy formation paradigm. Giant elliptical galaxies at z = 0 must have assembled rapidly, possibly within few 100 Myr through an extreme growth phase at high-redshift, characterized by elevated star formation rates of several thousand solar masses per year distributed over concurrent, gas-rich mergers. We present a novel view of the z = 4.3 protocluster core SPT2349–56 from sensitive multicycle Atacama Large Millimeter/submillimeter Array dust continuum and [C ii ]158 μ m line observations. Distributed across 60 kpc, a highly structured gas reservoir with a line luminosity of L [C II] = 3.0 ± 0.2 × 10 9 L ⊙ and an inferred cold gas mass of M gas = 8.9 ± 0.7 × 10 9 M ⊙ is found surrounding the central massive galaxy triplet. Like “beads on a string,” the newly discovered [C ii ] streamers fragment into a few kiloparsec-spaced and turbulent clumps that have a similar column density as local Universe spiral galaxy arms at Σ gas = 20–60 M ⊙ pc −2 . For a dust temperature of 30 K, the [C ii ] emission from the ejected clumps carries ≳3% of the far-IR luminosity, translating into an exceptionally low mass-to-light ratio of α [CII] = 2.95 ± 0.3 M ⊙ L ⊙ − 1 , indicative of shock-heated molecular gas. In phase space, about half of the galaxies in the protocluster core populate the same caustic as the [C ii ] streamers ( r / r vir × ∣Δ v ∣/ σ vir ≈ 0.1), suggesting angular momentum dissipation via tidal ejection while the brightest cluster galaxy (BCG) is assembling. Our findings provide new evidence for the importance of tidal ejections of [C ii ]-bright, shocked material following multiple major mergers that might represent a landmark phase in the z ≳ 4 coevolution of BCGs with their hot, metal enriched atmospheres.

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.

Contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé, mais le titre doit être comparé manuellement.

Titre Crossref
Bright [C <scp>II</scp> ]158 <i>μ</i> m Streamers as a Beacon for Giant Galaxy Formation in SPT2349-56 at <i>z</i> = 4.3
Date Crossref
10/02/2026
Éditeur
American Astronomical Society
Type
journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude et ne compte pas comme une seconde source scientifique indépendante.

Sujets associés

Galaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysical ResearchAstrophysics and Star Formation Studies

BNTIC News n’est pas le producteur de ces données. Recherche à la demande dans Crossref, OpenAIRE, DOAJ, Europe PMC, HAL, DataCite, ROR et la Banque mondiale, sans clé ; OpenAlex reste optionnel. Aucun service payant requis, aucune donnée externe enregistrée en base. Sources et limites.