Results 111 to 120 of about 739 (176)
Evidence for Environmental Effects in the z = 4.3 Protocluster Core SPT2349–56
We present Atacama Large Millimeter/submillimeter Array observations of the [C I ] 492 and 806 GHz fine-structure lines in 25 dusty star-forming galaxies (DSFGs) at z = 4.3 in the core of the SPT2349–56 protocluster.
Chayce Hughes +18 more
doaj +1 more source
JWST’s First Glimpse of a z > 2 Forming Cluster Reveals a Top-heavy Stellar Mass Function
Clusters and their progenitors (protoclusters) at z ∼ 2 − 4, the peak epoch of star formation, are ideal laboratories to study the formation process of both the clusters themselves and their member galaxies.
Hanwen Sun +13 more
doaj +1 more source
We present a selection of candidates of clusters and protoclusters of galaxies identified in the photometric data of the HSC-SSP Wide Public Data Release 3 (PDR3), spanning the redshift range 0.1 ≤ z ≤ 2. The selection method, detailed in Vicentin et al.,
Marcelo C. Vicentin +4 more
doaj +1 more source
Kingdom-wide analysis of the evolution of the plant type III polyketide synthase superfamily. [PDF]
Naake T +4 more
europepmc +1 more source
Natural product biosynthetic potential reflects macroevolutionary diversification within a widely distributed bacterial taxon. [PDF]
Silva SG +4 more
europepmc +1 more source
ABSTRACT Simulations predict that the galaxy populations inhabiting protoclusters may contribute considerably to the total amount of stellar mass growth of galaxies in the early universe. In this study, we test these predictions observationally, using the Taralay protocluster (formerly PCl J1001+0220) at z ∼ 4.57 in the COSMOS field ...
Priti Staab +28 more
openaire +2 more sources
Kinematic Analysis of z = 4.3 Galaxies in the SPT2349–56 Protocluster Core
SPT2349−56 is a protocluster discovered in the 2500 deg ^2 South Pole Telescope (SPT) survey. In this paper, we study the kinematics of the galaxies found in the core of SPT2349−56 using high-resolution (1.55 kpc spatial resolution at z = 4.303 ...
Aparna Venkateshwaran +12 more
doaj +1 more source
Nonlinear compositional and morphological evolution of ion irradiated GaSb prior to nanostructure formation. [PDF]
Lively MA +4 more
europepmc +1 more source
Studies of galaxy protoclusters yield insights into galaxy cluster formation complementary to those obtained via `archaeological' studies of present-day galaxy clusters. Submillimetre-selected galaxies (SMGs) are one class of sources used to find high-redshift protoclusters.
Araya-Araya, Pablo +8 more
openaire +2 more sources
The Timescales of Embedded Star Formation as Observed in STARFORGE
Star formation occurs within dusty molecular clouds that are then disrupted by stellar feedback. However, the timing and physical mechanisms that govern the transition from deeply embedded to exposed stars remain uncertain.
Tobin M. Wainer +9 more
doaj +1 more source

