Results 1 to 10 of about 108,957 (118)
Application of a Low-dissipation HLLD Approximate Riemann Solver to Solar Wind Simulations
We investigate the steady-state solar wind in spherical coordinates using a low-dissipation Harten–Lax–van Leer-Discontinuities Riemann solver, in which the magnetic field is decomposed into an initial potential field B _0 and a time-dependent part B _1 .
Caixia Li +3 more
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HDO Ice Detected toward an Isolated Low-mass Protostar with JWST
Water is detected in environments representing every stage of star and solar system formation, but its chemical evolution throughout these stages remains poorly constrained.
Katerina Slavicinska +17 more
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We report the detection of the [O iii ] auroral line in 42 galaxies within the redshift range of 3 < z < 10. These galaxies were selected from publicly available JWST data releases, including the JADES and PRIMAL surveys, and observed using both the low ...
Priyanka Chakraborty +12 more
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Element Nucleosynthetic Origins from Abundance Spatial Distributions beyond the Milky Way
An element’s astrophysical origin should be reflected in the spatial distribution of its abundance, yielding measurably different spatial distributions for elements with different nucleosynthetic sites.
Zefeng Li +9 more
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Quiescent prominences are large magnetic structures hosting cool plasma in surrounding million-degree solar coronae. Prominences host different flows that may distort magnetic field lines, which may lead to magnetic reconnection inside the prominence ...
Sandeep K. Dubey +2 more
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Theoretical and numerical simulations of black hole hot accretion flows have shown the ubiquitous existence of winds and predicted their properties, such as velocity and mass flux.
Fangzheng Shi +3 more
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We present initial results from extremely well-resolved 3D magnetohydrodynamical simulations of idealized galaxy clusters, conducted using the AthenaPK code on the Frontier exascale supercomputer.
Philipp Grete +7 more
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Constraining Resolved Extragalactic R21 Variation with Well-calibrated ALMA Observations
CO(1–0) and CO(2–1) are commonly used as bulk molecular gas tracers. The CO line ratios (especially CO(2–1)/CO(1–0)– R _21 ) vary within and among galaxies, yet previous studies on R _21 and alike often rely on measurements constructed by combining data ...
Jakob den Brok +15 more
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The Chemical Yields of Stars in the Mass Range 9–15 M⊙
In M. Limongi et al. we presented and discussed the main evolutionary properties and final fate of stars in the mass range 7−15 M _⊙ . The evolutions of those models were computed by means of a medium-sized nuclear network that guaranteed a proper ...
Marco Limongi +4 more
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Pivot of the Emerging Bipolar Magnetic Region in the Birth of Sigmoidal Solar Active Regions
We present an augmentation to long-standing evidence from observations and MHD modeling that (1) every solar emerging bipolar magnetic region (BMR) is made by an emerging Ω-loop flux rope, and (2) a twist in the flux-rope field makes the emerged field ...
Ronald L. Moore +5 more
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