Search Publications

Origin of the Unusual Composition of 3He-rich Solar Energetic Particles
DOI: 10.3847/1538-4357/adb48d Bibcode: 2025ApJ...981..178B

Wimmer-Schweingruber, Robert F.; Rodríguez-Pacheco, Javier; Ho, George C. +3 more

We examine 3He-rich solar energetic particles (SEPs) detected on 2023 October 24–25 by Solar Orbiter at 0.47 au. Measurements reveal that heavy-ion enhancements increase irregularly with mass, peaking at S. C, and especially N, Si, and S, stand out in the enhancement pattern with large abundances. Except for 3He, heavy-ion sp…

2025 The Astrophysical Journal
SOHO SolarOrbiter 0
3D Nonequilibrium Ionization and Spectroscopic Modeling of Coronal Mass Ejections. I. Comparison with Hinode/EIS Observations
DOI: 10.3847/1538-4357/ada7e8 Bibcode: 2025ApJ...980...30W

Landi, E.; Manchester, W. B.; Wraback, E. M. +1 more

High-resolution EUV spectroscopy provides an informative diagnostic tool for the early evolution of coronal mass ejections (CMEs) since it can directly measure many physical properties of CME plasma close to the Sun that cannot be determined from white-light coronagraphs or narrowband imagers. The Hinode/EUV Imaging Spectrometer (EIS) captured a s…

2025 The Astrophysical Journal
Hinode 0
Hydrostatic Equilibrium Constraints in X-COP Galaxy Clusters: Testing Hyperconical Modified Gravity in Hot-gas-dominated Regions
DOI: 10.3847/1538-4357/adb723 Bibcode: 2025ApJ...981..195M

Monjo, Robert

Modified Newtonian dynamics (MOND) was originally proposed to model galaxy rotation curves without dark matter. However, MOND presents difficulties in explaining the radial acceleration relation observed in galaxy clusters, and moreover, it does not completely eliminate the need for dark matter, since it requires using nonluminous particles (e.g.,…

2025 The Astrophysical Journal
XMM-Newton 0
The Origins of Lithium Enhancement in Polluted White Dwarfs
DOI: 10.3847/1538-4357/ad9a6d Bibcode: 2025ApJ...979..111K

Blouin, Simon; Dufour, Patrick; Clemens, J. Christopher +4 more

The bulk abundances of exoplanetesimals can be measured when they are accreted by white dwarfs. Recently, lithium from the accretion of exoplanetesimals was detected in relatively high levels in multiple white dwarfs. There are presently three proposed hypotheses to explain the detection of excess lithium in white dwarf photospheres: Big Bang and …

2025 The Astrophysical Journal
Gaia 0