Results 161 to 170 of about 636,610 (341)
The Evolution of Molecular Clouds: Turbulence-regulated Global Radial Collapse
The star formation efficiency (SFE) measures the proportion of molecular gas converted into stars, while the star formation rate (SFR) indicates the rate at which gas is transformed into stars.
An-Xu Luo, Hong-Li Liu, Jin-Zeng Li
doaj +1 more source
Star formation rates in normal and peculiar galaxies
Richard B. Larson, B. M. Tinsley
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The Scale‐dependent Energy Transfer Rate as a Tracer for Star Formation in CosmologicalN‐Body Simulations [PDF]
M. Hoeft, J. P. Mücket, P. Heide
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Comprehensive analysis of genomic mutations, gene expression, DNA methylation, and pathway analysis of TCGA data was carried out to define cancer types in which proteasome subunits expression is associated with worse survival. Albeit the effect of specific proteasome subunits on cellular function, the main role of the proteasome is better evaluated ...
Ruba Al‐Abdulla+5 more
wiley +1 more source
Determination of ADP/ATP translocase isoform ratios in malignancy and cellular senescence
The individual functions of three isoforms exchanging ADP and ATP (ADP/ATP translocases; ANTs) on the mitochondrial membrane remain unclear. We developed a method for quantitatively differentiating highly similar human ANT1, ANT2, and ANT3 using parallel reaction monitoring. This method allowed us to assess changes in translocase levels during cellular
Zuzana Liblova+18 more
wiley +1 more source
There is a broad consensus from theory that stellar feedback in galaxies at high redshifts is essential to their evolution, alongside conflicting evidence in the observational literature about its prevalence and efficacy.
Jack E. Birkin+25 more
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This nationwide study evaluated KRAS and NRAS mutations in 10 754 Turkish patients with metastatic colorectal cancer. The results revealed a mutation frequency of 51.1%, with 46.6% having KRAS mutations, 4.5% having NRAS mutations, and 48.5% being wild‐type for both.
Gozde Kavgaci+6 more
wiley +1 more source
Effects of Bursty Star Formation on [C ii] Line Intensity Mapping of High-redshift Galaxies
Bursty star formation—a key prediction for high-redshift galaxies from cosmological simulations explicitly resolving stellar feedback in the interstellar medium—has recently been observed to prevail among galaxies at redshift z ≳ 6.
Lun-Jun Liu+4 more
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Photometric redshifts in theHubble Deep Fields: evolution of extinction and the star formation rate [PDF]
M. Rowan-Robinson
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