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- What Does 2D Coronal Seismology Measure?
- Can Magnetic Reconnection Accelerate Energetic Particles in the Heliosheath?
- Constraints on the r-process Delay Time from Dwarf Spheroidal Galaxies
- Testing, Comparing, and Validating an L1 Method for Abundances Derivations from EUV Spectra
- An ALMA View on Molecular Complexity: Water, Methanol, and Methyl Formate in the HD 100546 and IRS 48 Disks
- The JADES Mass–Metallicity and Fundamental Metallicity Relations at z ≳ 2 Using New High-redshift Metallicity Calibrations
- The 2015–2017 Large EVPA Rotation in OJ 287: Dominant Propagating Component in a Helical Magnetic Field with Time-dependent Viewing Geometry
- Three-dimensional Magnetohydrodynamic Shocks and Associated Plasma Heating in the Solar Atmosphere
- Discovery of a 62 minute Long-period Transient with Near-orthogonal Rotator Geometry
- Exploring Magnetic Reconnection in a Sub-A-class Microflare Using Data-constrained Numerical Simulation and Multi-instrument Observations
- Eight New Ultramassive Black Hole Masses Confirm Best Correlation with Galaxy Core Sizes
- Dynamical Impacts of Accretion Streamers on Protoplanetary Disks
- ID-MAGE. II. The Star-forming Satellites of Low-mass Hosts
- Tidal Encounters of Close White Dwarf Binaries with Spinning Black Holes
- Solar Wind and PUI Proton Heating Rates and Turbulence Effects on Energetic Particles in the Heliosphere
- New Detections of H2CO and c-C3H2 in Planetary Nebulae: Broadening the Organic Inventory
- Extension of 2-Ethoxyethanol Rotational Spectroscopy and Its Search in the Interstellar Medium
- DZ White Dwarfs from HETDEX: New Identifications and Reclassifications
- The Relation between Magnetic-field Intensity and Size of the Emission Region in the High-synchrotron-peaked BL Lacertae Object Mrk 421
- Collisionless Electron Heat Flux for the Nonequilibrium Solar Wind Plasma: Revisiting Hollweg’s Parameter
- When the Shadow Meets Its Measure: Assessing the Feasibility of Submillimeter Black Hole Shadow Imaging in Megamaser-disk Active Galactic Nuclei
- Detection of HNCOH+ in the interstellar medium
- The clouds in the 'middle ages'. I. Star formation history and chemical abundances in the LMC
- Effects of Alfvénicity on the compressible energy cascade in magnetohydrodynamic solar-wind turbulence: Evidence from Parker Solar Probe, Solar Orbiter, and WIND observations
- Robustness of C/O and mean molecular weight under disequilibrium chemistry