Results 51 to 60 of about 10,106 (229)
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
On the Electromagnetic Energy Flow Along Geodesics
Abstract We present a field‐theoretic framework for modeling electromagnetic energy propagation in heterogeneous media by introducing the concept of electromagnetic geodesics. Unlike traditional ray optics, which assumes either a straight‐line propagation or a simple bending in refractive media, our approach formulates wave propagation as geodetic ...
Jacob T. Fokkema, Peter M. van den Berg
wiley +1 more source
We present new high-resolution ( R ∼ 114,000), near-ultraviolet spectra in the direction of 36 nearby (
Azmain H. Nisak +4 more
doaj +1 more source
X-ray Emission from the Interstellar and Circumgalactic Medium of Elliptical Galaxies based on MACER simulations [PDF]
Aditi Vijayan +4 more
openalex +1 more source
The chemistry of H2NC in the interstellar medium and the role of the C + NH3 reaction [PDF]
M. Agundez +5 more
openalex +1 more source
Science of omics: a molecular space odyssey
Experimental Physiology, EarlyView.
Salomé Coppens +3 more
wiley +1 more source
Theoretical Spectroscopic Study of Isopropyl Alcohol (CH3-CHOH-CH3)
Accurate spectroscopic parameters of isopropyl alcohol, a volatile organic compound present on Earth and in extraterrestrial atmospheres, are provided.
Mohammed Salah +3 more
doaj +1 more source
Peptide Bonds in the Interstellar Medium: Facile Catalytic Formation from Nitriles on Water-Ice Grains. [PDF]
Kerkeni B, Simmie JM.
europepmc +1 more source
Composition and quantities of dust produced by AGB-stars and returned to the interstellar medium [PDF]
A. S. Ferrarotti, H. P. Gail
openalex +1 more source
There is now abundant observational evidence that star formation is a highly dynamical process that connects filament hierarchies and supernova feedback from galaxy-scale kiloparsec filaments and superbubbles to giant molecular clouds (GMCs) on 100 pc ...
Bo Zhao +4 more
doaj +1 more source

