Atomic Hydrogen in Distant Galaxies

Resonance ◽  
2021 ◽  
Vol 26 (7) ◽  
pp. 919-938 ◽  
Author(s):  
Nissim Kanekar ◽  
Aditya Chowdhury ◽  
Jayaram N. Chengalur
Keyword(s):  
Atomic Hydrogen ◽  
Distant Galaxies

Longitudinal electronic and nuclear spin diffusion in atomic hydrogen

1985 ◽  
Vol 46 (8) ◽  
pp. 1335-1344 ◽  
Author(s):  
J.P. Bouchaud ◽  
C. Lhuillier
Keyword(s):  
Nuclear Spin ◽  
Atomic Hydrogen ◽  
Spin Diffusion

PHOTONS SHEDDING LIGHT UPON CHARGE EXCHANGE PROCESSES IN COLLISIONS OF 24 keV O3+ WITH ATOMIC HYDROGEN

1989 ◽  
Vol 50 (C1) ◽  
pp. C1-349-C1-352
Author(s):  
R. HOEKSTRA ◽  
K. BOORSMA ◽  
F. J . de HEER ◽  
R. MORGENSTERN
Keyword(s):  
Charge Exchange ◽  
Atomic Hydrogen ◽  
Exchange Processes

The First Galaxies in the Universe

2013 ◽  
Author(s):  
Abraham Loeb ◽  
Steven R. Furlanetto
Keyword(s):  
Galaxy Evolution ◽  
Big Bang ◽  
First Stars ◽  
Distant Galaxies ◽  
Formation And Evolution ◽  
Early Galaxies ◽  
First Galaxies ◽  
Large Telescopes ◽  
New Generation ◽  
The Big Bang

This book provides a comprehensive, self-contained introduction to one of the most exciting frontiers in astrophysics today: the quest to understand how the oldest and most distant galaxies in our universe first formed. Until now, most research on this question has been theoretical, but the next few years will bring about a new generation of large telescopes that promise to supply a flood of data about the infant universe during its first billion years after the big bang. This book bridges the gap between theory and observation. It is an invaluable reference for students and researchers on early galaxies. The book starts from basic physical principles before moving on to more advanced material. Topics include the gravitational growth of structure, the intergalactic medium, the formation and evolution of the first stars and black holes, feedback and galaxy evolution, reionization, 21-cm cosmology, and more.

Radiative and Hydrodynamical Model of a Steady Shock Wave in Atomic Hydrogen

2009 ◽  
Author(s):  
Giuliano D'Ammando ◽  
Daniela Pietanza ◽  
Gianpiero Colonna ◽  
Savino Longo ◽  
Mario Capitelli
Keyword(s):  
Shock Wave ◽  
Atomic Hydrogen ◽  
Hydrodynamical Model ◽  
Steady Shock

Atomic Hydrogen - A Reagent for the Extraction of Chemical Species from Silicon Surfaces

1992 ◽  
Author(s):  
Jr. Yates ◽  
Cheng J. T. ◽  
Gao C. C. ◽  
Colaianni Q. ◽  
Choyke M. L. ◽  
...  
Keyword(s):  
Atomic Hydrogen ◽  
Chemical Species ◽  
Silicon Surfaces

Acetylene chemisorption at palladium: Effect of temperature and structure of the surface

1984 ◽  
Vol 49 (6) ◽  
pp. 1448-1458
Author(s):  
Josef Kopešťanský
Keyword(s):  
Work Function ◽  
Atomic Hydrogen ◽  
Effect Of Temperature ◽  
Thermally Stable ◽  
Template Effect ◽  
Temperature Range ◽  
Adsorbed Layers ◽  
Different Types ◽  
Adsorption Complexes ◽  
Low Coverage

The effect of temperature and structure of the palladium surfaces on acetylene chemisorption was studied along with the interaction of the adsorbed layers with molecular and atomic hydrogen. The work function changes were measured and combined with the volumetric measurements and analysis of the products. At temperature below 100 °C, acetylene is adsorbed almost without dissociation and forms at least two different types of thermally stable adsorption complexes. Acetylene adsorbed at 200 °C is partly decomposed, especially in the low coverage region. Besides the above mentioned effects, the template effect of adsorbed acetylene was studied in the temperature range from -80° to 25 °C. It has been shown that this effect is a typical phenomenon of the palladium-acetylene system which is not due to surface impurities.

New Particles

2018 ◽  
Author(s):  
Roger H. Stuewer
Keyword(s):  
Gamma Rays ◽  
Atomic Hydrogen ◽  
Nuclear Physics ◽  
Hydrogen Isotope ◽  
Alpha Particles ◽  
Cloud Chamber ◽  
Ernest Rutherford ◽  
James Chadwick ◽  
Theoretical Foundations ◽  
New Particles

In December 1931, Harold Urey discovered deuterium (and its nucleus, the deuteron) by spectroscopically detecting the faint companion lines in the Balmer spectrum of atomic hydrogen that were produced by the heavy hydrogen isotope. In February 1932, James Chadwick, stimulated by the claim of the wife-and-husband team of Irène Curie and Frédéric Joliot that polonium alpha particles cause the emission of energetic gamma rays from beryllium, proved experimentally that not gamma rays but neutrons are emitted, thereby discovering the particle whose existence had been predicted a dozen years earlier by Chadwick’s mentor, Ernest Rutherford. In August 1932, Carl Anderson took a cloud-chamber photograph of a positron traversing a lead plate, unaware that Paul Dirac had predicted the existence of the anti-electron in 1931. These three new particles, the deuteron, neutron, and positron, were immediately incorporated into the experimental and theoretical foundations of nuclear physics.

Atomic Hydrogen and Star Formation in the Bridge/Ring Interacting Galaxy Pair NGC 7714/7715 (Arp 284)

1997 ◽  
Vol 483 (2) ◽  
pp. 754-766 ◽  
Author(s):  
Beverly J. Smith ◽  
Curtis Struck ◽  
Richard W. Pogge
Keyword(s):  
Star Formation ◽  
Atomic Hydrogen
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