Results 131 to 140 of about 716,854 (348)
The stellar masses of ~40 000 UV selected galaxies from the WiggleZ survey at 0.3 [PDF]
We characterize the stellar masses and star formation rates in a sample of ∼40 000 spectroscopically confirmed UV-luminous galaxies at 0.3 5σ in the UKIDSS-LAS at all redshifts.
M. Banerji +26 more
semanticscholar +1 more source
The stellar mass-radius relation is determined by using new data on absolute dimensions of the components of well-detached binary systems. The relation is compared with the published empirical and theoretical mass-radins relations. The location of the knee in the empirical relation is estimated in 1.66 solar mass.
openaire +2 more sources
Fetal Brain Tumor Harboring a Unique ROCK1::BRAF Fusion
Pediatric Blood &Cancer, EarlyView.
Marllon Cindra Sant'Ana +8 more
wiley +1 more source
In this study, we found that human cervical‐derived adipocytes maintain intracellular iron level by regulating the expression of iron transport‐related proteins during adrenergic stimulation. Melanotransferrin is predicted to interact with transferrin receptor 1 based on in silico analysis.
Rahaf Alrifai +9 more
wiley +1 more source
Stochasticity in Star Clusters: Reduced Random Sampling Method
This paper aims to contribute to the debate taking place nowadays on the two extreme schemes of sampling the stellar masses within star clusters, known as Optimal Sampling and Random Sampling.
de Meulenaer P. +3 more
doaj +1 more source
Pop III Stellar Masses and IMF
We provide a status report on our current understanding of the mass scales for Pop III.1 and Pop III.2 stars. Since the last review (Norman 2008), substantial progress has been made both numerically and analytically on the late stages of protostellar ...
Norman, Michael L.
core +1 more source
AME - Asteroseismology Made Easy. Estimating stellar properties by use of scaled models [PDF]
We present a new method to obtain stellar properties for stars exhibiting solar-like oscillations in an easy, fast, and transparent way. The method, called Asteroseismology Made Easy (AME), can determine stellar masses, mean-densities, radii, and surface
Aguirre, V. Silva +2 more
core +1 more source
DYNAMICAL VERSUS STELLAR MASSES IN COMPACT EARLY-TYPE GALAXIES: FURTHER EVIDENCE FOR SYSTEMATIC VARIATION IN THE STELLAR INITIAL MASS FUNCTION [PDF]
Several independent lines of evidence suggest that the stellar initial mass function (IMF) in early-type galaxies becomes increasingly “bottom-heavy” with increasing galaxy mass and/or velocity dispersion, σ.
C. Conroy +4 more
semanticscholar +1 more source
Tau acetylation at K331 has limited impact on tau pathology in vivo
We mapped tau post‐translational modifications in humanized MAPT knock‐in mice and in amyloid‐bearing double knock‐in mice. Acetylation within the repeat domain, particularly around K331, showed modest increases under amyloid pathology. To test functional relevance, we generated MAPTK331Q knock‐in mice.
Shoko Hashimoto +3 more
wiley +1 more source
In the third APOKASC catalog, we present data for the complete sample of 15,808 evolved stars with APOGEE spectroscopic parameters and Kepler asteroseismology.
Marc H. Pinsonneault +40 more
doaj +1 more source

