Results 151 to 160 of about 157,333 (319)
Anatomy of the Star Formation in a Tidally Disturbed Disk Galaxy: NGC 3718
The Astrophysical JournalWe present a UV, optical, and near-IR study of the star-forming complexes in the nearby peculiar galaxy NGC 3718, using Ultraviolet Imaging telescope, Galaxy Evolution Explorer, Spitzer, and DECam Legacy Survey imaging data.
Chandan Watts +2 more
doaj +1 more source
Dynamical Models for the Formation and Evolution of Spherical Galaxies [PDF]
, 1974 Richard B. Larson
openalex +1 more source
Limnology and Oceanography, EarlyView.Abstract Diatom‐dominated blooms in coastal upwelling systems contribute disproportionately to global primary production. The fate of carbon captured during a diatom bloom is often influenced by species‐specific ecological differences. However, successional patterns that take place during a diatom bloom are often oversimplified, and the diversity of ...
Joseph H. Vineis +3 more
wiley +1 more source
A Review of Recent Observations of Galactic Winds Driven by Star Formation
Galaxies, 2018 Galaxy-scale outflows of gas, or galactic winds (GWs), driven by energy from star formation are a pivotal mechanism for regulation of star formation in the current model of galaxy evolution.
David S. N. Rupke
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The evolving disk galaxy population
, 2008 In this contribution, I present a simplified overview of the evolution of the disk galaxy population since z=1, and a brief discussion of a few open questions.
Bell, Eric F.
core
Macromolecular Rapid Communications, EarlyView.Multidrug resistant Pseudomonas (P.) aeruginosa is detected in many infected wounds and is challenging to treat with antibiotics. As an alternative, this work incorporates anti‐P. aeruginosa Neko phages into electrospun fibres to explore their potential for treating infected wounds.
Tian Ju +7 more
wiley +1 more source
Chemical evolution of galaxies and galaxy formation mechanisms [PDF]
Proceedings of Baryons in Dark Matter Halos — PoS(BDMH2004), 2004 I will describe the results if models for the chemical evolution of galaxies of different morphological type (ellipticals, spirals and irregulars), and compare them with observations in order to impose constraints on the mechianisms of formation and evolution of galaxies.
openaire +2 more sources
Homochiral Self‐Sorting During Macrocycle Formation and their Chiroptical Properties
ChemistryOpen, EarlyView.Imine condensation of C2‐symmetric chiral aldehydes with aliphatic amines results in 2 : 2 macrocycles lacking self‐sorting, whereas aromatic amines yield macrocycles with complete homochiral self‐sorting. These macrocycles exhibit unique chiroptical properties attributed to rigidification compared to the starting aldehydes.
Diptiprava Sahoo, Soumen De
wiley +1 more source
5–25 μm Galaxy Number Counts from Deep JWST Data
The Astrophysical JournalGalaxy number counts probe the evolution of galaxies over cosmic time and serve as a valuable comparison point to theoretical models of galaxy formation.
Meredith A. Stone +7 more
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EPJ Web of Conferences, 2018 This contribution deals with the important subject of the nucleosynthesis of heavy elements in the Galaxy. After an overview of several observational features, the physical processes responsible mainly for the formation of heavy elements will be ...
El Eid Mounib F.
doaj +1 more source