Results 71 to 80 of about 2,568,324 (143)
Atomic Power Development Associates Report APDA-124 [PDF]
, 1960 Report describing the Enrico Fermi Atomic Power Plant, its fast breeder reactor, and heat transport ...
Atomic Power Development Associates
core
15 yr of Interstellar Neutral Hydrogen Observed with the Interstellar Boundary Explorer
The Astrophysical Journal Supplement SeriesThe interactions of our heliosphere with the surrounding local interstellar medium (LISM) lead to a range of observable phenomena such as energetic neutral atoms (ENAs) from the boundary regions of the heliosphere and the influx of interstellar neutrals (
André Galli +13 more
doaj +1 more source
Structure and Spectroscopy of Criegee Intermediates in Gas‐ and Aqueous Environments
Helvetica Chimica Acta, Volume 109, Issue 5, May 2026.ABSTRACT The dynamics and spectroscopy of the small (H2COO) and large (CH3CHOO) Criegee intermediates (CIs) in the gas phase, inside/on water droplets, on amorphous solid water (ASW) and in bulk water are investigated using validated energy functions.
Cangtao Yin +2 more
wiley +1 more source
Atomic Energy Commission Report AECD-3792
, 1955 Report discussing the progress of various projects at the Knolls Atomic Power Laboratory during the period from March to May ...
Knolls Atomic Power Laboratory
core
Simulating molecular cloud regulated star formation in Galaxies [PDF]
, 2007 This thesis is primarily concerned with understanding the process of galaxy formation via the simulation of the interstellar medium, star formation and supernova feedback.
Booth, Craig Martin
core
Observed Timescales of Stellar Feedback in Star-forming, Low-mass Galaxies
The Astronomical JournalUnderstanding the timescales of atomic gas turbulence is crucial to understanding the interplay between star formation and the interstellar medium (ISM). To investigate the timescales of turbulence low-mass galaxies (10 ^6.8
Laura Congreve Hunter +7 more
doaj +1 more source
Novel algorithms for the understanding of the chemical cosmos [PDF]
, 2015 Molecular data from the interstellar medium (ISM) contain information that holds the key to understanding our chemically controlled cosmos and to unlocking the secrets of our universe.
Makrymallis, A
core
The H i Reservoir in Central Spiral Galaxies and the Implied Star Formation Process
The Astrophysical Journal LettersThe cold interstellar medium (ISM) as the raw material for star formation is critical to understanding galaxy evolution. It is generally understood that galaxies stop making stars when, in one way or another, they run out of gas. However, here we provide
Jing Dou +16 more
doaj +1 more source
Atomic Energy Commission Report TID-7546 Book 1
, 1958 Preface: The Fuel Elements Conference held in Paris, France, November 18 to 23, 1957, under the joint sponsorship of the U.S. Atomic Energy Commission and the French Commissarat à l'Energie Atomique (CEA), provided an intensive review of fuel-element ...
U.S. Atomic Energy Commission
core
Cool Dark Gas in Cygnus X: The First Large-scale Mapping of Low-frequency Carbon Recombination Lines
The Astrophysical JournalUnderstanding the transition from atomic gas to molecular gas is critical to explain the formation and evolution of molecular clouds. However, the gas phases involved, cold H i and CO-dark molecular gas, are challenging to directly observe and physically
Kimberly L. Emig +16 more
doaj +1 more source