Results 1 to 10 of about 12,196 (218)
Evolution of slow electrostatic shock into a plasma shock mediated by electrostatic turbulence
The collision of two plasma clouds at a speed that exceeds the ion acoustic speed can result in the formation of shocks. This phenomenon is observed not only in astrophysical scenarios, such as the propagation of supernova remnant (SNR) blast shells into
M E Dieckmann +4 more
doaj +1 more source
The A2Π–X2Σ+ Band System of ScO for M-type Star Spectral Analysis
M-type stars are the most abundant stars in our Galaxy. Their visible spectra are characterized by strong TiO and VO absorption bands with occasional ScO bands near 6000–6100 Å.
Léo Lavy +2 more
doaj +1 more source
Molecules in Cool Stars: The A2Π − X2Σ+ and the B2Σ+ − X2Σ+ Band Systems of CaCl
Cool red giant stars exhibit absorption bands of calcium monochloride (CaCl) in the optical region. In this work, the bands of CaCl corresponding to the A ^2 Π − X ^2 Σ ^+ transition with ${v}^{{\prime} }\leqslant $ 4 and v ″ ≤ 4, and B ^2 Σ ^+ − X ^2 Σ ^
Léo Lavy, Peter F. Bernath
doaj +1 more source
Functionalization of Benzene Ices by Atomic Oxygen
Small aromatic molecules, including functionalized derivatives of benzene, are known to be present throughout the different stages of star and planet formation.
Elettra L. Piacentino +8 more
doaj +1 more source
ELI-Beamlines (ELI-BL), one of the three pillars of the Extreme Light Infrastructure endeavour, will be in a unique position to perform research in high-energy-density-physics (HEDP), plasma physics and ultra-high intensity (UHI) (1022W/cm2) laser–plasma
S. Weber +39 more
doaj +1 more source
Atomic Data for Nonequilibrium Modeling of Kilonovae: The Ionization Properties of Te I–III
Kilonovae, the electromagnetic transients produced from two merging neutron stars, exhibit evolving spectral signatures in ultraviolet, visible, and infrared radiation.
S. J. Bromley +7 more
doaj +1 more source
Design of experiments characterizing heat conduction in magnetized, weakly collisional plasma
Heat conduction in weakly collisional, magnetized plasma is challenging to model accurately due to multifaceted physics governing heat-carrying electrons, including microinstabilities that scatter electrons and modify heat transport.
Thomas A. Vincent +17 more
doaj +1 more source
Ultra-high charge electron acceleration for nuclear applications
Ultra-intense laser-plasma wakefield accelerator possess several superior properties compared with the traditional radio-frequency accelerators. These characteristics include femtosecond duration, micro-source size, and ultra-dense beam density, result ...
Liming Chen +8 more
doaj +1 more source
Broad band high resolution rotational spectroscopy for Laboratory Astrophysics. [PDF]
Cernicharo J +35 more
europepmc +1 more source
Reverse-Engineering Laboratory Astrophysics: Oxygen Inner-shell Absorption in the ISM. [PDF]
García J +4 more
europepmc +1 more source

