Most stars form in multiple systems, with profound implications in numerous astronomical phenomena intrinsically linked to multiplicity. However, our knowledge about the process of how multiple stellar systems form is incomplete and biased toward nearby ...
Qiu-yi Luo +16 more
doaj +1 more source
Genomic Analysis of the Rare Slightly Halophilic Myxobacterium "Paraliomyxa miuraensis" SMH-27-4, the Producer of the Antibiotic Miuraenamide A. [PDF]
Liu Y, Ojika M.
europepmc +1 more source
Identification of Galaxy Protoclusters Based on the Spherical Top-hat Collapse Theory
We propose a new method for finding galaxy protoclusters that is motivated by structure formation theory and also directly applicable to observations. We adopt the conventional definition that a protocluster is a galaxy group whose virial mass M _vir < M
Jaehyun Lee +9 more
doaj +1 more source
Forming intracluster gas in a galaxy protocluster at a redshift of 2.16. [PDF]
Di Mascolo L +15 more
europepmc +1 more source
A Survey of Sulfur-bearing Molecular Lines toward the Dense Cores in 11 Massive Protoclusters
Sulfur-bearing molecules are commonly detected in dense cores within star-forming regions, but the total sulfur budget is significantly lower when compared to the interstellar medium value.
Mengyao Tang +8 more
doaj +1 more source
The One-hundred-deg2 DECam Imaging in Narrowbands (ODIN): Survey Design and Science Goals
We describe the survey design and science goals for One-hundred-deg ^2 DECam Imaging in Narrowbands (ODIN), a NOIRLab survey using the Dark Energy Camera (DECam) to obtain deep (AB ∼ 25.7) narrowband images over an unprecedented area of sky.
Kyoung-Soo Lee +42 more
doaj +1 more source
Visualization of tumor heterogeneity and prediction of isocitrate dehydrogenase mutation status for human gliomas using multiparametric physiologic and metabolic MRI. [PDF]
Hagiwara A +13 more
europepmc +1 more source
Galaxy protocluster candidates around z ~ 2.4 radio galaxies
We study the environments of 6 radio galaxies at 2.2 < z < 2.6 using wide-field near-infrared images. We use colour cuts to identify galaxies in this redshift range, and find that three of the radio galaxies are surrounded by significant surface overdensities of such galaxies.
Hatch, N. +12 more
openaire +4 more sources
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

