Results 141 to 150 of about 60,296 (295)
There are more things in heaven and Earth than we dream of in our physiology
The Journal of Physiology, EarlyView.
Victor A. Maltsev +2 more
wiley +1 more source
ABSTRACT This review explores the impact of gravitational instability on convective heat transfer, integrating existing research results and theoretical models. Gravitational instability is vital in promoting or hindering convective actions in different systems, such as atmospheric events, ocean currents, and industrial processes.
Hossam A. Nabwey +3 more
wiley +1 more source
On the Evolutionary History of a Simulated Disk Galaxy as Seen by Phylogenetic Trees
Phylogenetic methods have long been used in biology and more recently have been extended to other fields—for example, linguistics and technology—to study evolutionary histories.
Danielle de Brito Silva +14 more
doaj +1 more source
Galactic chemical evolution in hierarchical formation models - I. Early-type galaxies in the local Universe [PDF]
Matías Arrigoni +3 more
openalex +1 more source
Assessing the validity of leucine zipper constructs predicted by AlphaFold
Abstract AP‐1 transcription factors are a network of cellular regulators that combine in different dimer pairs to control a range of pathways involved in differentiation, growth, and cell death. They dimerize via leucine zipper coiled‐coil domains that are preceded by a basic DNA binding domain.
Isobel Mitic +4 more
wiley +1 more source
Quantifying Bursty Star Formation in Dwarf Galaxies
Dwarf galaxy star formation histories are theoretically expected to be bursty, potentially leaving distinct imprints on their chemical evolution. We propose that episodic starbursts with quiescent periods longer than ~100 Myr should lead to discontinuous
Yuan-Sen Ting, Alexander Ji
doaj +1 more source
Galaxy Formation and Chemical Evolution in Hierarchical Hydrodynamical Simulations [PDF]
S. A. Cora +3 more
openalex +1 more source
Adsorption of Helium on Cationic or Anionic Tetracene and Pentacene
How does the arrangement of helium atoms that are adsorbed on tetracene or pentacene ions change with increasing coverage? When does the adsorption layer change from 1D to 2D, and to 3D? Is the transition abrupt? Are the helium atoms localized? Is the arrangement the same for cations and anions? What changes as the acene grows in length?
Miriam Kappe +6 more
wiley +1 more source

