Solar & stellar physics
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- Testing Models of Disk Formation and Gravito-Viscous Evolution Against Observations of Young Protoplanetary Disks
- Extreme Hard X-ray Variability in the TeV Blazar Mrk 421: Insights from NuSTAR Observations
- Formation and Evolution of [Wolf-Rayet] Planetary Nebulae through a Late Thermal Pulse
- Clumps in a Cocoon: Geometry and Mixing Set the Universal X-ray to Hα Surface Brightness Ratio
- DOWSING, Dust Observations With SCUBA-2 In Nearby Galaxies: I. Dust in M 81
- Effect of tidal gravity and planetary rotation on the retrieved atmospheric abundances of close-in exoplanets
- Orientation of the spin axes of large Kuiper belt bodies as an indicator of the mechanism of their origin
- CACOFONI: Cosine Amplitude Calibration Organized in Frequency for On-sky Nimble Interaction-matrix. A Novel Method for Calibrating Adaptive Optics Systems II
- No Evidence for a Supermassive Black Hole Binary in GSN 069
- NGC 3227 Blinks: An Extreme Changing-look Event in a Seyfert Galaxy
- Multilobed Stokes V Profiles of the Fe i 407.17 nm Line Observed by Sunrise iii
- “Mega-Earths” are Likely an Artifact of Stellar Activity
- SN 2023fyq: Direct detection of a Type Ibn supernova progenitor and its multiwavelength environmental constraints
- RIOJA: The dusty outflows and density-complex interstellar medium in the N-enhanced lensed galaxy RXCJ2248-ID at z = 6.1
- A transmission hologram for slitless spectrophotometry on a convergent telescope beam
- SOLACE: A Contrastive Learning Framework for Predicting Solar Proton Events and Geomagnetic Storms from Flare–Coronal Mass Ejection Events
- Revisiting Ca II Activity Indices in FGK Stars: Systematic Biases in Infrared Triplet Measurements
- Satellite Streaks in HETDEX: Spectra, Orbital Identification, and Survey Impact
- Validation of Habitable Zone Limits with a New Radiative–Convective Equilibrium Climate Model
- Saturn’s Evolutionary History and Seismology: Survival of Deep Stably Stratified Regions in Evolutionary Models of Saturn Consistent with Ring Seismology
- 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