Results 261 to 270 of about 3,407 (289)
Abstract A core drilled through shocked and faulted Archean granitoid gneisses and dolerites in the eroded peak ring of the 70–80 km diameter Morokweng impact structure intersects multiple centimeter‐ to meter‐wide clastic‐matrix breccias containing a polymict clast population of lithic and mineral clasts and altered, millimeter‐ to centimeter ‐size ...
Roger L. Gibson +3 more
wiley +1 more source
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: The hidden circumgalactic medium. [PDF]
Lee M +31 more
europepmc +1 more source
X-ray astronomy from the lunar surface. [PDF]
Gandhi P.
europepmc +1 more source
Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback
Eckert D +21 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Cosmic Rays and Galactic Winds
Astrophysics and Space Science, 2004Repeated SN-explosion provide large amounts of thermal energy as well as energetic particles through a 1. order Fermi-process. Both effects together with the generation of AlfveŽn-waves are considered to drive a large scale outflow from a galaxy. These so-called galactic winds transport stellar material enriched by heavy elements into the intergalactic
exaly +2 more sources
Galactic winds: a short review
Astrophysics and Space Science, 2007Galactic winds are important in recycling energy and metals in galaxies. They are also suspected to be the primary mechanism in the enrichment of the intergalactic medium. New observations are revealing the ubiquity of galactic winds, particularly at high redshift. We review the observational evidence for them in nearby star-forming and active galaxies
Joss Bland-Hawthorn +2 more
exaly +2 more sources
Galactic winds in dwarf galaxies
New Astronomy Reviews, 2007Abstract Galactic winds are mayor ingredients of our current paradigms of galaxy formation and evolution. They are needed to explain the chemical evolution of galaxies and the intergalactic medium, the luminosity function of galaxies, the formation of galaxies, and the reionization of the universe, just to name a few topics.
Dominik J Bomans +2 more
exaly +2 more sources
Kontext: Untersuchung der Charakteristika von galaktischen Winden bei Simulation von multiplen Supernovaexplosionen. Weiters wird der Einfluss von Diffusion untersucht. Ziele: Zeitlich versetzten Supernova-Explosionen führt zur Ausbildung von multiplen Schockwellen.
E. A. Dorfi, D. Breitschwerdt
core +3 more sources

