Results 121 to 130 of about 665 (145)

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Resolving the hot and ionized Universe through the Sunyaev-Zeldovich effect. [PDF]

Open Res Eur
Di Mascolo L, Perrott Y, Mroczkowski T, Raghunathan S, Andreon S, Ettori S, Simionescu A, van Marrewijk J, Cicone C, Lee M, Nelson D, Sommovigo L, Booth M, Klaassen P, Andreani P, Cordiner MA, Johnstone D, van Kampen E, Liu D, Maccarone TJ, Morris TW, Orlowski-Scherer J, Saintonge A, Smith M, Thelen AE, Wedemeyer S.   +25 more
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Using wavelet decomposition to determine the dimension of structures from projected images. [PDF]

Proc Natl Acad Sci U S A
Mayboroda S, Spergel DN.
europepmc   +1 more source

The photometry and kinematics studies of NGC 2509 derived from Gaia DR3. [PDF]

Sci Rep
Ahmed NM, Tadross AL.
europepmc   +1 more source

The IMAP Magnetometer. [PDF]

Space Sci Rev
Horbury TS, O'Brien HL, Greenaway C, Roberts A, Crabtree A, Tomes M, Facchinelli M, Finlayson M, Bharatia M, Fauchon-Jones E, Tapley M, Pope S, Jones D, Richter I, Dalla S, Russell C, Schwadron NA, Gkioulidou M, McComas DJ.   +18 more
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Study of the amorphization process of MgSiO3 by ion irradiation as a form of dust processing in astrophysical environments

Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, 2002
Abstract The study of the crystalline-to-amorphous transition of silicates triggered by ion irradiation is useful for the understanding of the structural modification of interstellar dust grains. We focused our experiments on the mineral enstatite (MgSiO3), an essential part of the polycrystalline silicate dust.
F. Schrempel, C. Jäger, D. Fabian, J. Dorschner, Th. Henning, W. Wesch   +5 more
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Physical properties of clusters relevant for the dust formation process in oxygen-rich astrophysical environments

2003
The formation of small solid particles (dust grains) from the gas phase in the circumstellar environments of evolved stars or the atmospheres of substellar objects (brown dwarfs) requires suitable physical and chemical conditions. The temperature and density of the gas have to be confined to a certain regime, the emph{dust formation window}, in order ...
openaire   +2 more sources

Influence of non-spherical dust grains on the growing of astrophysical dusty plasma waves with (r, q) distribution function

Astroparticle Physics, 2020
Myoung-Jae Lee, Young-Dae Jung, Naoko Ashikawa   +2 more
exaly  

Ice Coverage of Dust Grains in Cold Astrophysical Environments

Physical Review Letters, 2020
, Thomas Henning, Alexey Potapov
exaly  

Carbonaceous dust grains seen in the first billion years of cosmic time

Nature, 2023
Santiago Arribas, Renske Smit, Pierre Ferruit   +2 more
exaly  

Residue from vacuum ultraviolet irradiation of benzene ices: Insights into the physical structure of astrophysical dust

Spectrochimica Acta - Part A: Molecular and Biomolecular Spectroscopy, 2020
Bhalamurugan Sivaraman, Nigel John Mason, E Shivakarthik   +2 more
exaly