Results 31 to 40 of about 2,752,786 (196)

Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars

Universe, 2021
Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy.
Chemseddine Ananna, Francesco Barile, Axel Boeltzig, Carlo Giulio Bruno, Francesca Cavanna, Giovanni Francesco Ciani, Alessandro Compagnucci, Laszlo Csedreki, Rosanna Depalo, Federico Ferraro, Eliana Masha, Denise Piatti, David Rapagnani, Jakub Skowronski   +13 more
doaj   +1 more source

Radiative Shocks in Astrophysics and the Laboratory [PDF]

Astrophysics and Space Science, 2005
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
openaire   +2 more sources

Laboratory Astrophysics White Paper [PDF]

, 2006
Laboratory astrophysics and complementary theoretical calculations are the foundations of astronomical and planetary research and will remain so for many generations to come. From the level of scientific conception to that of the scientific return, it is
Federman, Steve, Salama, Farid, Brickhouse, Nancy, Stancil, Phillip, Weingartner, Joe, Ziurys, Lucy, Savin, Daniel Wolf, Kwong, Victor   +7 more
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Formation of dense, electromagnetically accelerated plasma for laboratory astrophysics

EPJ Web of Conferences, 2013
We proposed tapered pinch discharge as a measure to conduct laboratory astrophysics experiments. Basic behaviors of the plasma have been characterized using a prototype device. Results show that the plasma flux and velocity depend on initial gas density,
Adachi K., Nakajima M., Kawamura T., Horioka K.   +3 more
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Table-top solar flares produced with laser driven magnetic reconnections

EPJ Web of Conferences, 2013
The American Nuclear Society (ANS) has presented the prestigious Edward Teller award to Dr. Bruce A. Remington during the 2011 IFSA conference due to his “pioneering scientific work in the fields of inertial confinement fusion (ICF), and especially ...
Zhong J.Y., Li Y.T., Wang X.G., Wang J.Q., Dong Q.L., Liu X., Lin X.X., Yuan D.W., Du F., Wang S.J., Zhang L., An L., Xiao C.J., Wei H.G., Zhang K., Wang F.L., Jiang S.E., Ding Y.K., Cao Z.R., Yuan Z., Zhang H.Y., Yang Z.W., Zhu J.Q., He X.T., Cai H.B., Zhao G., Zhang J.   +26 more
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Bombardment of CO Ice by Cosmic Rays. I. Experimental Insights into the Microphysics of Molecule Destruction and Sputtering

The Astrophysical Journal, 2023
We present a dedicated experimental study of microscopic mechanisms controlling radiolysis and sputtering of astrophysical ices upon bombardment by cosmic-ray ions.
Alexei V. Ivlev, Barbara M. Giuliano, Zoltán Juhász, Péter Herczku, Béla Sulik, Duncan V. Mifsud, Sándor T. S. Kovács, K. K. Rahul, Richárd Rácz, Sándor Biri, István Rajta, István Vajda, Nigel J. Mason, Sergio Ioppolo, Paola Caselli   +14 more
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Astronomy & Astrophysics (CAUCASUS)-VOLUME 2

, 2020
The second volume of the international scientific journal Astronomy & Astrophysics (Caucasus) contains the scientific works delivered as scientific reports by their authors at International Scientific Conference Modern Problems of Astrophysics – II ...
(CAUCASUS), Astronomy & Astrophysics
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Cryogenic Differential Calorimetry: Exothermicity of Amorphous-to-crystalline Phase Transitions (ACPT) in Astrophysical and Cometary Ice Analogs

The Astrophysical Journal
Amorphous ice is understood to be the predominant phase of water in cometary nuclei. A significant number of other volatiles can be trapped in amorphous H _2 O ice and released during the amorphous-to-crystalline phase transition (ACPT).
Rahul K. Kushwaha, Murthy S. Gudipati, Bryana L. Henderson   +2 more
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Nuclear astrophysics in the laboratory and in the universe

AIP Advances, 2014
Nuclear processes drive stellar evolution and so nuclear physics, stellar models and observations together allow us to describe the inner workings of stars and their life stories.
A. E. Champagne, C. Iliadis, R. Longland
doaj   +1 more source

The Laboratory Astrophysics Spectroscopy Programme at Imperial College London

Galaxies, 2018
Accurate atomic parameters, such as transition probabilities, wavelengths, and energy levels, are indispensable for the analysis of stellar spectra and the obtainment of chemical abundances.
María Teresa Belmonte, Juliet C. Pickering, Christian P. Clear, Florence Concepción Mairey, Florence Liggins   +4 more
doaj   +1 more source