Results 111 to 120 of about 105,573 (267)
Cosmic-Ray Induced Diffuse Emissions from the Milky Way and Local Group Galaxies
Cosmic rays fill up the entire volume of galaxies, providing an important source of heating and ionisation of the interstellar medium, and may play a significant role in the regulation of star formation and galactic evolution.
Abdo +5 more
core +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
Shocks in the Very Local Interstellar Medium. [PDF]
Mostafavi P +12 more
europepmc +1 more source
Possible interaction of interstellar particles with the solar and terrestrial environment [PDF]
The possibility for detection of interstellar particles in the earth's environment is considered on the basis of the passage of the solar system through the interstellar medium.
Greenberg, J. M.
core +1 more source
The Solar Magnetic Hump, Heliopause, and the Very Local Interstellar Medium
The magnetic hump was observed from 2020.4 to ∼2022 by Burlaga et al. who offered the hypothesis that it originated at the Sun during the declining phase of the solar cycle.
L. F. Burlaga +4 more
doaj +1 more source
Gas-phase formation of the resonantly stabilized 1-indenyl (C9H7•) radical in the interstellar medium. [PDF]
Yang Z +9 more
europepmc +1 more source
Pulsar distances, spiral structure and the interstellar medium [PDF]
B. Y. Mills
openalex +1 more source
The interstellar medium of our Galaxy [PDF]
The development of our understanding of the gaseous component of the interstellar medium is reviewed. During the 20th century our picture of diffuse material in space has grown from a simple model of isolated clouds in thermal equilibrium with stellar radiation fields to one of a richly varied composite of materials with a wide range of physical ...
openaire +3 more sources
Advancing our understanding of astrophysical turbulence is bottlenecked by the limited resolution of numerical simulations that may not fully sample scales in the inertial range.
Diane M. Salim +2 more
doaj +1 more source
Observations of the Outer Heliosphere, Heliosheath, and Interstellar Medium. [PDF]
Richardson JD +5 more
europepmc +1 more source

