Results 51 to 60 of about 11,541,392 (252)
Mass observation / by Mass Observation.
Electronic reproduction. Canberra, A.C.T.
Mass-Observation.
core
Initial mass function of intermediate-mass black hole seeds [PDF]
We study the initial mass function (IMF) and hosting halo properties of intermediate-mass black holes (IMBHs, 104-6 M⊙) formed inside metal-free, UV-illuminated atomic-cooling haloes (virial temperature Tvir ≥ 104 K) either via the direct collapse of the
Ferrara, A. +9 more
core +2 more sources
CT10 regulator of kinase (CRK) and CRK‐Like (CRKL) are signaling adaptors driving cell adhesion, motility, differentiation, and proliferation. SH2‐domain containing (SH) proteins are enriched in YXXP motifs which when phosphorylated create preferred binding sites for CRK family SH2 domains.
Phoebe M. Cousens +8 more
wiley +1 more source
Going Public in Poland: Case-by-Case Privatizations, Mass Privatization and Private Sector Initial Public Offerings [PDF]
This study compares the characteristics and the price behavior of case-by-case privatization initial public offerings, private sector initial public offerings and the mass privatization program in Poland over the first eight years after the reopening of ...
Wolfgang Aussenegg
core
The process of internalization of the Shiga toxin A subunit via formation of a complex with the Shiga toxin B subunit, which specifically binds to the Gb3 receptor. The peptide is designed to act as a carrier of drugs into cancer cells. Here, we explored the potential of peptides derived from the catalytic A subunit of Shiga toxin (STxA) to be drug ...
Giulia Opassi +6 more
wiley +1 more source
Self-regulated galaxy evolution within a self-consistently varying galaxy-wide initial mass function
Context. Semi-analytical evolution models of galaxies are a useful and computationally inexpensive tool for a fast assessment of individual properties and their evolution. In this work, specifically the influence of a metallicity- and star-formation-rate-
Hof Lukas +3 more
doaj +1 more source
Theories of the initial mass function
We review the various theories which have been proposed along the years to explain the origin of the stellar initial mass function. We pay particular attention to four models, namely the competitive accretion and the theories based respectively on ...
Gilles Chabrier +3 more
core +1 more source
Variations in integrated galactic initial mass functions due to sampling method and cluster mass function [PDF]
Context. Stars are thought to be formed predominantly in clusters. The star clusters are formed according to a cluster initial mass function (CMF) similar to the stellar initial mass function (IMF). Both the IMF and the CMF can be approximated by (broken)
Astrophysics +5 more
core +1 more source
Conserved binding mode but diverse interfaces of MreC‐PBP2 interactions
The crystal structure of abMreC reveals a conserved two β‐barrel architecture and provides structural insights into its role within the bacterial elongasome. The abMreC–abPBP2 complex model identifies the molecular basis of MreC‐mediated PBP2 recognition, contributing to the regulation of peptidoglycan synthesis.
Hyunseok Jang +4 more
wiley +1 more source
Among the most important ways to investigate galaxies' distribution over cosmic time is the luminosity function LF in terms of baryonic disc mass ψS(Mb), magnitude .
Al Najm M.N. +2 more
doaj +1 more source

